<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">
    wjnst
   </journal-id>
   <journal-title-group>
    <journal-title>
     World Journal of Nuclear Science and Technology
    </journal-title>
   </journal-title-group>
   <issn pub-type="epub">
    2161-6795
   </issn>
   <issn publication-format="print">
    2161-6809
   </issn>
   <publisher>
    <publisher-name>
     Scientific Research Publishing
    </publisher-name>
   </publisher>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="doi">
    10.4236/wjnst.2024.144013
   </article-id>
   <article-id pub-id-type="publisher-id">
    wjnst-137109
   </article-id>
   <article-categories>
    <subj-group subj-group-type="heading">
     <subject>
      Articles
     </subject>
    </subj-group>
    <subj-group subj-group-type="Discipline-v2">
     <subject>
      Engineering, Physics 
     </subject>
     <subject>
       Mathematics
     </subject>
    </subj-group>
   </article-categories>
   <title-group>
    Proposal of a Deuterium-Deuterium Fusion/PWR Fission Hybrid Reactor
   </title-group>
   <contrib-group>
    <contrib contrib-type="author" xlink:type="simple">
     <name name-style="western">
      <surname>
       Patrick
      </surname>
      <given-names>
       Lindecker
      </given-names>
     </name>
    </contrib>
   </contrib-group> 
   <aff id="affnull">
    <addr-line>
     aIndependent Researcher, Paris, France
    </addr-line> 
   </aff> 
   <pub-date pub-type="epub">
    <day>
     29
    </day> 
    <month>
     09
    </month>
    <year>
     2024
    </year>
   </pub-date> 
   <volume>
    14
   </volume> 
   <issue>
    04
   </issue>
   <fpage>
    190
   </fpage>
   <lpage>
    233
   </lpage>
   <history>
    <date date-type="received">
     <day>
      6,
     </day>
     <month>
      September
     </month>
     <year>
      2024
     </year>
    </date>
    <date date-type="published">
     <day>
      28,
     </day>
     <month>
      September
     </month>
     <year>
      2024
     </year> 
    </date> 
    <date date-type="accepted">
     <day>
      28,
     </day>
     <month>
      October
     </month>
     <year>
      2024
     </year> 
    </date>
   </history>
   <permissions>
    <copyright-statement>
     © Copyright 2014 by authors and Scientific Research Publishing Inc. 
    </copyright-statement>
    <copyright-year>
     2014
    </copyright-year>
    <license>
     <license-p>
      This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/
     </license-p>
    </license>
   </permissions>
   <abstract>
    This article proposes to associate a Deuterium-Deuterium (D-D) fusion reactor with a PWR (fission Pressurized Water Reactor) in a hybrid reactor. Even if the mechanical gain (Q factor) of the D-D fusion reactor is below the unity and consequently consumes more energy than it supplies, due to the high energy amplification factor of the PWR fission reactor, the global yield is widely superior to 1. As the energy supplied by the fusion reactor is relatively low and as the neutrons supplied are mainly issued from D-D fusions (at 2.45 MeV), the problems of heat flux and neutrons damage connected with materials, as with D-T fusion reactors are reduced. Of course, there is no need to produce Tritium with this D-D fusion reactor. This type of reactor is able to incinerate any mixture of natural Uranium, natural Thorium and depleted Uranium (waste issued from enrichment plants), with natural Thorium being the best choice. No enriched fuel is needed. So, this type of reactor could constitute a source of energy for several thousands of years because it is about 90 more efficient than a standard fission reactor, such as a PWR or a Candu one, by extracting almost completely the energy from the fertile materials U238 and Th232. For the fission part, PWR technology is mature. For the fusion part, it is based on reasonable hypotheses done on present Stellarators projects. The working of this reactor is continuous, 24 hours a day. In this paper, it will be targeted a reactor able to provide a net electric power of about 1400 MWe, as a big fission power plant.
   </abstract>
   <kwd-group> 
    <kwd>
     Fusion Reactor
    </kwd> 
    <kwd>
      Fission Reactor
    </kwd> 
    <kwd>
      Hybrid Reactor
    </kwd> 
    <kwd>
      Nuclear Energy
    </kwd> 
    <kwd>
      Deuterium-Deuterium Reactor
    </kwd> 
    <kwd>
      Deuterium
    </kwd> 
    <kwd>
      Colliding Beams
    </kwd> 
    <kwd>
      Racetrack
    </kwd> 
    <kwd>
      Stellarator
    </kwd> 
    <kwd>
      Power Plant
    </kwd> 
    <kwd>
      PWR
    </kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <sec id="s1">
   <title>1. Introduction</title>
   <sec id="s1_1">
    <title>1.1. Goal, Presentation and Notations Used</title>
    <p>The goal of this article is to describe a hybrid power plant formed by:</p>
    <p>All these beams, initially directed axially, circulate inside a figure of “0” configuration, also called a Stellarator “racetrack”. The global injected current is nil. This reactor would produce nuclear fusions with a mechanical gain (Q), i.e., fusion power/mechanical injection power, depending on the pipe radius (Rp) superior to 1 in <xref ref-type="bibr" rid="scirp.137109-1">
      [1]
     </xref> but inferior to 1 for this hybrid reactor. For example, at Rp = 2 m, Q = 0.184, versus Q &gt; 10 for a D-T Stellarator of the same radius, as, for example, the Helias 5-B project.</p>
    <p>Note that in the standard way, the plasma is formed and heated with different devices (Joule effect, radio frequencies, adiabatic compression, neutral atoms injection…) and not by opposite beams. However, the best way to form and heat the plasma is outside of the goal of this article.</p>
    <p>These fusion and fission reactors are completely independent of one another, i.e., an evolution on the fission reactor, as the reactivity or the temperature has no impact on the fusion reactor.</p>
    <p>It is reminded that Deuterium (D) and Tritium (T) are hydrogen isotopes comprising, besides one proton, either one neutron (Deuterium) or two neutrons (Tritium).</p>
    <p>The problems of cryogenic systems, ultra-high vacuum, particle diversion in the “Divertor” (to “clear” plasma), radiation hygiene, possible instabilities, and way to realize toroidal and poloidal fields are not addressed in this paper.</p>
    <p>This article is only concerned with the fusion and fission aspects, at the level of principles, the physics used to be relatively simple.</p>
    <p>The main goal of this article is to propose a physical model of this hybrid reactor. A small program called “D_D_PWR_hybrid_reactor” (§1.5), based on the model developed in <xref ref-type="bibr" rid="scirp.137109-1">
      [1]
     </xref> and in this article, is proposed with its Delphi 6 source code. Thanks to this model, any D-D/PWR hybrid reactor can be roughly designed.</p>
    <p>It is obvious that the reactor presented in this paper would be rather large for practical realization, i.e., 200 m long according to §2.1. To reduce the size of such a reactor, one can increase the Beta factor (§3.2) if possible or, more slightly, the maximum K_eff (§4.5).</p>
    <p>Interest of such hybrid reactor</p>
    <p>The interest of such a reactor is that the source of energy could last a very long time. Below are the explanations of why.</p>
    <p>First, about the Deuterium, a m<sup>3</sup> of sea water contains 32.4 g of Deuterium (D2). So, the reserve of Deuterium would last millions (see billions) of years (see <xref ref-type="bibr" rid="scirp.137109-1">
      [1]
     </xref> for details).</p>
    <p>Besides the important stock of depleted Uranium, there are two natural materials that can be incinerated in this hybrid reactor: the natural Uranium and the natural Thorium.</p>
    <p>Moreover, the possible stock of enriched Uranium and the stock of Plutonium issued from reprocessing plants for nuclear waste could be slowly incinerated (for example, mixed with depleted Uranium or with natural Thorium), but they are not taken into account in this document as the available quantities of these materials are not important.</p>
    <p>The conventional Uranium reserve, at less than 130 $/kg in 2021, is equal to 6,078,500 tons (from <xref ref-type="bibr" rid="scirp.137109-3">
      [3]
     </xref>). Moreover, 1.2 million tons of depleted Uranium (at about 0.3% of U235) are also available (from <xref ref-type="bibr" rid="scirp.137109-3">
      [3]
     </xref>).</p>
    <p>The Thorium reserve, at less than 80 $/kg in 2016, is equal to 6,355,000 tons (from <xref ref-type="bibr" rid="scirp.137109-4">
      [4]
     </xref>).</p>
    <p>Using the proposed hybrid reactor in its default configuration, it is found that the net electrical energy produced by one ton of:</p>
    <p>The world electric energy consumption is equal to 29471 TWh in 2023, according to <xref ref-type="bibr" rid="scirp.137109-5">
      [5]
     </xref> (p. 15), with 29471 TWh equivalent to 1.0609E20 J.</p>
    <p>Now, let’s suppose that all the electricity produced in the world is supplied by plants using the type of hybrid reactor proposed in this paper. In this case and neglecting the O<sub>2</sub>, the consumption of electricity would be covered for:</p>
    <p>The total makes 1984 years. Now, it must be taken into account that the conventional and unconventional reserves of natural Uranium are much larger than the value given above. For example, see the reference <xref ref-type="bibr" rid="scirp.137109-6">
      [6]
     </xref> (p. 94). The time during which Uranium and Thorium could supply all the world electricity would rather be about 8900 years. This is calculated without taking into account the unconventional reserves of Thorium.</p>
    <p>Moreover, a part of the heat produced by these reactors could be used without being transformed into electricity for heating networks, desalination plants, etc.</p>
    <p>Comparison with the Candu and PWR fission reactors</p>
    <p>The Candu reactor uses natural Uranium up to an average burn-up of 7.5 GWd/t. A standard PWR uses enriched Uranium at 3.4% up to a burn-up of about 42 GWd/t. This ton of enriched Uranium is obtained from 7 tons of natural Uranium at 0.7% of U235, leaving 6 tons of depleted Uranium at 0.25% of U235 as waste. Reported to the ton of natural Uranium, the burn-up is equal to 42/7 = 6 GWd/t. Let’s say that thanks to certain improvements and the use of MOX fuel, the average burn-up grows up to 7.5 GWd/t as for the Candu.</p>
    <p>In the reactor object of this article, the burn-up of the consumed fuel is very high: 723 GWd/t for natural Uranium and 819 GWd/t for natural Thorium, so close to the maximum possible. Hence, this reactor is 723/7.5 = 96 times more efficient that a standard reactor (PWR or Candu). Now, these values of burn-up must be considered as a bit optimistic because the fuel evolution taken into account (§4.12) is simplified, so the efficiency gain is certainly a bit lower, but not much below 96.</p>
    <p>Notations and units</p>
    <p>In a formula, the × and / operations take precedence over the + and − operations, for example:</p>
    <p>
     <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
       <mi>
         A 
       </mi> 
       <mo>
         × 
       </mo> 
       <mi>
         B 
       </mi> 
       <mo>
         + 
       </mo> 
       <mi>
         C 
       </mi> 
       <mo>
         × 
       </mo> 
       <mi>
         D 
       </mi> 
       <mo>
         = 
       </mo> 
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          ( 
        </mo> 
        <mrow> 
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           A 
         </mi> 
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           × 
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          ) 
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         + 
       </mo> 
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        </mo> 
        <mrow> 
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         </mo> 
         <mi>
           D 
         </mi> 
        </mrow> 
        <mo>
          ) 
        </mo> 
       </mrow> 
      </mrow> 
     </math>.</p>
    <p>The comma is a figure separator. For example: “100,000” means a hundred thousand.</p>
    <p>SI units, multiples and sub-multiples (cm particularly) are only used, with the exception of the “eV” (“electronVolt”), which is a unit of energy quantity used in the particles domain, i.e., 1 eV is equivalent to 1.60219E−19 J. It is the potential energy of a single charge submitted to a potential of 1 V.</p>
    <p>Note that “We” means “W” (watt) for electrical power.</p>
    <p>The fuel burn-up is expressed in “MWd/t”, i.e., “Thermal energy in MW for one day per ton of fuel”. 1 MWd is equivalent to 1E6 × 3600 × 24 = 8.64E10 J. It is sometimes used “GWd/t” rather than “MWd/t”, with</p>
    <p>1 GWd/t = 1000 MWd/t.</p>
   </sec>
   <sec id="s1_2">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>1.2. Quick Hybrid Reactor Historic and Comparison with the Option Explored in This Document</title>
    <p>The hybrid fusion-fission reactor concept dates from the 1950s. At the end of the 70s, a hybrid D-T tokamak/fission reactor was envisaged, but the provisional cost was considered dissuasive.</p>
    <p>For example, the problem of a blanket providing fissions and breeding Tritium was (and remains) complex to solve: if a neutron is used to breed Tritium via a reaction with Li6, this neutron is not used for fission, and reversely. In addition, Lithium must be separated from water due to an exothermic reaction between both.</p>
    <p>Fusion devices using a Deuterium beam at high energy (1.5 MeV) were also envisaged as a source of neutrons for a fission reactor.</p>
    <p>In 1979, Hans A. Bethe defended in <xref ref-type="bibr" rid="scirp.137109-7">
      [7]
     </xref> this type of hybrid D-T tokamak/fission reactor.</p>
    <p>In 1993, Carlos Rubbia and his team proposed <xref ref-type="bibr" rid="scirp.137109-8">
      [8]
     </xref> to use, instead of a D-T fusion reactor, a beam of protons at high energy (1 GeV) hitting a heavy metallic target (lead, for example) which produces, by spallation, the necessary neutrons to breed the fissile materials.</p>
    <p>Since then, many configurations have been proposed, including “Stellarators as fusion-fission reactor candidates” in <xref ref-type="bibr" rid="scirp.137109-9">
      [9]
     </xref> (p. 195), for example.</p>
    <p>In all cases, as the fission reactor is in a sub-critical configuration, hybrid reactors can be called “energy amplifiers” because the fission reactor multiplies the number of neutrons generated by the fusion reactor or by spallation and generates fissions at about 200 MeV with neutrons at high energy (14.06 MeV for the D-T reactors). If the source of neutrons stops, the fissions generated in the fissile materials quickly stop. However, as in a standard fission reactor, after a stop, the fission reactor must be cooled due to the residual heat produced by fission products.</p>
    <p>About experimentation, the T-15 MD tokamak will explore the feasibility of a hybrid fusion/fission model. See <xref ref-type="bibr" rid="scirp.137109-10">
      [10]
     </xref>.</p>
    <p>The option explored in this article is the use, rather than a D-T fusion reactor, of a D-D fusion reactor, using a “racetrack” Stellarator, in which neutrons breed a sub-critical PWR. The advantage is relative simplicity, as there is no need for Tritium. Moreover, the proportion of high-energy neutrons at 14.06 MeV is low. So even if the mechanical gain Q of a D-D reactor is low and even if the reactivity of a PWR is low with natural Uranium or Thorium, the energy amplification remains sufficient due to the generation of relatively low energy neutrons (2.45 MeV) for thermal fissions at about 200 MeV.</p>
   </sec>
   <sec id="s1_3">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>1.3. Methods of the Work</title>
    <p><u>Step 1</u>: the global working of the proposed D-D/PWR hybrid reactor is first described at the level of principle in §2.</p>
    <p><u>Step 2</u>: in §3 and §4, the fusion and the fission reactors are modeled using classical formulas of physics. The previous fusion model developed in <xref ref-type="bibr" rid="scirp.137109-1">
      [1]
     </xref> is taken into account in the program, but it is not described, except for its modifications in §3. Only the fission part is described in this article (§4). The global working of the reactor is shown in §2.1.</p>
    <p><u>Step 3</u>: once the physical models are achieved, they will be used in §5 to estimate this reactor with several types of fuel. A discussion about results, points to deepen, improvements, and safety aspects follow. In §6, conclusions are drawn.</p>
   </sec>
   <sec id="s1_4">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>1.4. List of the Main Variables and Acronyms Used in This Article</title>
    <p><u>Below are the main variables used </u><u>in </u><u>the article (local variables are not listed)</u><u>:</u></p>
    <p>Beta Diamagnetism factor</p>
    <p>B Toroidal magnetic field (T)</p>
    <p>E_equi Equilibrium energy of the plasma in eV</p>
    <p>E_inj Energy of the injected Deuterium ions and electrons in eV</p>
    <p>K Neutrons multiplication factor (in K_infinite and K_eff)</p>
    <p>nD Deuterium ions density (number of Deuterium ions per m<sup>3</sup>)</p>
    <p>ne Electrons density (number of electrons per m<sup>3</sup>)</p>
    <p>pht Per hundred thousand, i.e., in 1/100,000</p>
    <p>QMechanical gain (i.e., fusion power/mechanical injection power), without dimension</p>
    <p>Rp Interior pipe radius (m) of the fusion reactor</p>
    <p><u>Below are the acronyms used:</u></p>
    <p>“D-D” for “Deuterium-Deuterium”</p>
    <p>“D-T” for “Deuterium-Tritium”</p>
    <p>“PWR” for “Pressurized Water Reactor”</p>
    <p>“UHV” for “Ultra High Vacuum”</p>
   </sec>
   <sec id="s1_5">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>1.5. “D_D_PWR_Hybrid_Reactor” Program Based on the Fusion and Fission Physical Models</title>
    <p>It proposed the program called “D_D_PWR_hybrid_reactor” V2.0, which implements the physical model described in this article (fission reactor), plus the one described in <xref ref-type="bibr" rid="scirp.137109-1">
      [1]
     </xref> (fusion reactor). The executable program with its Delphi 6 source code can be downloaded from this direct link: <xref ref-type="bibr" rid="scirp.137109-http://f6cte.free.fr/D_D_PWR_hybrid_reactor.zip">
      http://f6cte.free.fr/D_D_PWR_hybrid_reactor.zip
     </xref>. It is enough to paste this address into your Internet browser. Download the file. Create a folder (C:D_D_PWR_hybrid_reactor, for example), unzip the D_D_PWR_hybrid_reactor.zip file in it, and then start: C:D_D_PWR_hybrid_reactorD_D_PWR_hybrid_reactor.exe.</p>
    <p>In case of failure of this WEB address, this program will be available on the Zenodo WEB open repository by searching with the title of this article.</p>
    <p>
     <xref ref-type="fig" rid="fig1">
      Figure 1
     </xref> below is a snapshot of the program running the default configuration, the fuel being natural Uranium. It also appears the end of the results displayed on the black DOS window.</p>
    <sec id="s1">
     <title>2. Description of the Hybrid Reactor</title>
    </sec>
    <sec id="s2_6">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>2.1. Generalities</title>
     <p>It is composed of a fusion reactor all along the axis. It is surrounded by a fission reactor along both straight parts only, i.e., between A and D and B and C in <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>.</p>
     <p>About the half-toruses at each end of the reactor (A to B and D to C, in <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>), the two volumes between the beryllium wall and the 316LN wall don’t contain any fission reactor. About these two volumes:</p>
     <fig id="fig1" position="float">
      <label>Figure 1</label>
      <caption>
       <title>Figure 1. D-D/PWR Hybrid reactor V.2.0 program snapshot running its default configuration.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId15.jpeg?20241111100718" />
     </fig>
     <p>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>About both half-toruses at the level of the fusion part:</p>
     <p>Reversely, the necessary magnetic field for the straight parts is supposed to be simpler and to permit a circular pipe section.</p>
     <p>The fusion reactor is described in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>. It pertains to the “Colliding Beam Fusion Reactors” (CBFR) category of reactors. D+ ions and electrons are injected, at the same energy, with elevated currents up to the moment when the currents circulating in the figure of “0” reach their nominal values (the global current being nil). In permanent working, the electrons and the D+ ions are injected (at E_inj)</p>
     <fig id="fig2" position="float">
      <label>Figure 2</label>
      <caption>
       <title>Figure 2. D-D/PWR fusion reactor principle diagram.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId16.jpeg?20241111100719" />
     </fig>
     <p>at a rate permitting to cover losses and fusions so as to keep the beam neutral. The working of such D-D fusion reactor is continuous, 24 hours a day.</p>
     <p>In <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>, the principle diagram of this figure of “0” hybrid reactor is displayed. On this diagram, it appears stocky for representation necessity, but it is rather long and narrow: the overall height of the fusion reactor (H in <xref ref-type="fig" rid="fig3">
       Figure 3
      </xref>) is, in fact, 16.71 times larger than the width (W in <xref ref-type="fig" rid="fig3">
       Figure 3
      </xref>).</p>
     <p>Still in <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>, note that the thick 316LN exterior wall around the straight pipes (between A and D and B and C) corresponds to the metallic protection wall between the magnetic coils and the pressurized water.</p>
     <p>For a PWR, this wall would be called the “Reactor vessel body”. Note also that, to simplify, the core barrel around the fuel assemblies is not taken into account.</p>
     <p>At the level of the half-toruses, the 316LN exterior wall, jointly with the borated water, must provide the protection of the magnetic coils against heat and neutrons. Its thickness is supposed, a priori, to be the same as its thickness at the level of the straight parts, so 16.9 cm applies to the default configuration.</p>
     <p>The geometry of the fusion reactor is detailed in <xref ref-type="fig" rid="fig3">
       Figure 3
      </xref>.</p>
     <fig id="fig3" position="float">
      <label>Figure 3</label>
      <caption>
       <title>Figure 3. Geometry of the D-D fusion reactor on the YZ plane along the axis of the reactor.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId17.jpeg?20241111100719" />
     </fig>
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        </mfrac> 
        <mo>
          = 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            5 
          </mn> 
          <mo>
            × 
          </mo> 
          <mi>
            π 
          </mi> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          + 
        </mo> 
        <mn>
          1 
        </mn> 
        <mo>
          = 
        </mo> 
        <mn>
          16.71 
        </mn> 
       </mrow> 
      </math></p>
     <p>For the default configuration, Rp = 2 m, r = 6 m, L = 188.5 m, W = 12 m and H = 200.5 m.</p>
     <p>
      <xref ref-type="fig" rid="fig4">
       Figure 4
      </xref> shows, in a general way, how the hybrid reactor energy balance is taken into account, relatively to the power plant.</p>
     <p>The variables referred to the fusion reactor (Poutput, Pneu, PlostFi, PlostReactor, Pra, Q) are described in Appendix B of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
     <p>The global fusion power (Pth_fusion_W calculated in §3.4) is generated by the half-toruses and the straight lines. The volume of the straight lines being equal to 60/66 = 91% of the fusion volume, it will be supposed that 90% of Pth_fusion_W will reach the fission reactor and finally the water/steam circuit via the steam generators, so:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Psg_fusion_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          0.9 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Pth_fusion_W 
        </mtext> 
       </mrow> 
      </math> (2.1)</p>
     <p>If the heat power generated by the fission reactor is called Pth_fission_W (calculated in §4.6), the global power supplied to the steam generators will be equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Psg_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Psg_fusion_W 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Pth_fission_W 
        </mtext> 
       </mrow> 
      </math> (2.2)</p>
     <p>Note that the mechanical power provided by the primary coolant pumps (<xref ref-type="fig" rid="fig4">
       Figure 4
      </xref>) to the primary coolant is neglected in the energy balance. This power is normally added to the thermal power supplied to the steam generators (Psg_W).</p>
     <fig id="fig4" position="float">
      <label>Figure 4</label>
      <caption>
       <title>Figure 4. D-D/PWR hybrid reactor energy balance.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId36.jpeg?20241111100718" />
     </fig>
    </sec>
    <sec id="s2_7">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>2.2. Presentation and Working of the Fusion Reactor—Why This Type of Fusion Reactor</title>
     <p><u>Presentation and working of the fusion reactor (se</u><u>e </u><xref ref-type="bibr" rid="scirp.137109-1">
       <u>[1]</u>
      </xref> <u>for details))</u></p>
     <p>From an initial rectilinear movement, the behavior of the injected particles (<xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>) quickly becomes isotropic before thermalization. It is the proposed (but not exclusive) way to fill and heat the plasma.</p>
     <p>The Coulomb collisions between D+ ions and electrons permit a permanent exchange of energy between these particles. Plasma is heated, for a part, by fusion products: T+, p, He3+ and He4+ ions and maintained at an equilibrium energy E_equi. Replacement particles are injected at E_inj to replace lost particles and to heat the plasma.</p>
     <p>The toroidal magnetic field (B) must be axial relatively to the pipe and maximum to confine particles (electrons + ions). The present industrial maximum B limit for superconducting coils is 5 T (Tesla). So, this 5 T field will be supposed to be the default value.</p>
     <p>At fusion densities, a poloidal field is indispensable to limit the particle shift inside loops, particularly for the half-torus at each end of the reactor.</p>
     <p>The half-torus at each end of the reactor will only be considered in terms of the rate of energy loss, a loss which is more important than on straight pipes.</p>
     <p>There are mainly primary fusions between Deuterium nuclei, but also secondary fusions between Deuterium and Tritium nuclei and between Deuterium and Helium-3, as specified below.</p>
     <p>D+ + D+ → T+ (+1.01 MeV) + p (+3.03 MeV) (at 50%)</p>
     <p>D+ + D+ → He3+ (+0.82 MeV) + n (+2.45 MeV) (at 50%)</p>
     <p>D+ + T+ → He4+ (+3.52 MeV) + n (+14.06 MeV)</p>
     <p>D+ + He3+ → He4+ (+ 3.67 MeV) + p (+ 14.67 MeV) (aneutronic fusion).</p>
     <p>Note that at an equilibrium energy of about 29 keV, the Deuterium/Helium-3 fusions are very rare.</p>
     <p>In <xref ref-type="fig" rid="fig5">
       Figure 5
      </xref>, it is displayed the reactivities used in this paper for:</p>
     <p><u>Note</u>: the reactivity, written “&lt;σ x w&gt;”, is the integration of the product of the fusion cross-section σ by the relative speed w between particles over all the energies distributed according to the Maxwell-Boltzmann distribution, i.e., for a thermalized plasma.</p>
     <p>Note that, in general, the reactivities are displayed with the abscissa in temperature (in keV) and not in energy (in keV). The relationship is Energy (keV) = 1.5 x Temperature (keV)</p>
     <p>Contrary to the fission neutrons, which follow an energy spectrum, fusion neutrons have discrete values (2.45 MeV and 14.06 MeV). Both values can be exactly determined considering:</p>
     <fig id="fig5" position="float">
      <label>Figure 5</label>
      <caption>
       <title>Figure 5. Reactivities of the D-D/D-T/D-He3 fusions. The abscissa is the equilibrium energy (E_equi) in keV, and the ordinate is the reactivity in m<sup>3</sup>/s × 1E−23.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId37.jpeg?20241111100719" />
     </fig>
     <p><u>Why this type of fusion reactor</u></p>
     <p>A D-T reactor (as in <xref ref-type="bibr" rid="scirp.137109-2">
       [2]
      </xref>) could be proposed, as this one is able to supply energy with a mechanical gain superior to 10. But here, the fission reactor amplifies the neutron power by a factor of about 130 (depending on the configuration), so there is no need to look for high performance of the fusion reactor.</p>
     <p>The D-T reactor is complex due to the necessity to supply Tritium, which does not exist in nature.</p>
     <p>The neutrons generated by the D-T reactor are mainly of 14.06 MeV energy, which limits the energy amplification of the fission reactor compared to the 2.45 MeV energy from D-D fusions. Moreover, neutrons of 14.06 MeV energy drastically increase the problem on materials. So, a D-D reactor is preferable.</p>
     <p>Here, the D-D reactor is the one described in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> and modified in §3, working in a reasonable domain, i.e., with a Beta factor (cf. §3.2) equal or inferior to 0.05 which is the present limit for Stellarators, see <xref ref-type="bibr" rid="scirp.137109-14">
       [14]
      </xref> and <xref ref-type="bibr" rid="scirp.137109-15">
       [15]
      </xref>. But the mechanical gain Q is inferior to 1.</p>
     <p>Compared to a D-T reactor, the performance being weak, the neutrons flow and the average heat flow are relatively weak. Moreover, in the default configuration, only 26% of the neutrons have a 14.06 MeV energy. So, relatively to the Beryllium wall, the mechanical resistance in front of such neutron flow is not critical. The cooling of the Beryllium wall will not be a problem, the heat flux being widely inferior to 1 MW/m<sup>2</sup>, i.e., about 85 kW/m<sup>2</sup> at the straight parts level and about 420 kW/m<sup>2</sup> at the half-toruses level.</p>
     <p>Now, it will be more complicated at the level of the Divertor, where the heat flow is locally more important. However, it would be desirable to avoid Tungsten for the Divertor and to keep on with Beryllium, due to the possible erosion of Tungsten, which has a high atomic number that would cause a big loss by radiation.</p>
     <p>The proposed D-D fusion reactor is probably feasible with the present technology because it is much simpler than the D-T Stellarators projects such as the Helias one (<xref ref-type="bibr" rid="scirp.137109-11">
       [11]
      </xref>), as no Tritium must be supplied and the thermal and neutrons constraints are minimal (see §5.5).</p>
    </sec>
    <sec id="s2_8">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>2.3. Presentation and Working of the Fission Reactor—Why This Type of Fission Reactor</title>
     <p><u>Presentation and working of the fission reactor</u></p>
     <p>The fusion neutrons (mainly at 2.45 MeV but also at 14.06 MeV for a small part) issued from the straight pipes (see <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>) of the fusion reactor cross the beryllium inner wall (5 cm thickness) with very little loss. This flow of neutrons is amplified by the sub-critical fission reactions in the fuel (about 12 cm thickness of fuel rods). The amplification of energy is partly due to the ratio between the fission energy (about 200 MeV) and the neutron average kinetic power (about 5.4 MeV). The reflector is a layer of 20 cm thickness of water (about the thickness used on PWRs) which goal is to limit the neutron leak and to slow down neutrons. The 316LN non-magnetic stainless steel wall, with a thickness of 16.9 cm, withstands the pressure (69 bar gauge) and protects the magnetic coils against fission neutrons.</p>
     <p>The pressurized light water serves as a neutron decelerator, reflector and cooling fluid, transporting the heat produced in the fission reactor to the steam generators (see <xref ref-type="fig" rid="fig4">
       Figure 4
      </xref>).</p>
     <p><u>Why this type of fission reactor</u></p>
     <p>The main goal here is to have the most compact fission reactor so as to limit the mass of this reactor and the dimension of the super-conducting coils, even at the price of a small loss of reactivity. Moreover, this reactor must be able to incinerate natural Uranium and Thorium.</p>
     <p>The heavy water or graphite moderated reactors have a very good reactivity due to an excellent moderation, but they are very large and heavy.</p>
     <p>The BWR (Boiling Water Reactor) uses light water as PWR, but it is larger than the PWR due to a lower moderation power of the boiling water.</p>
     <p>The FNR (fast–neutron reactor) is compact, but it works on the fast spectrum of neutrons. So, with natural Uranium or Thorium, its reactivity would be too low.</p>
     <p>The best compromise solution for a fission reactor is the PWR, as it is compact and disposes of reasonable reactivity. This is due to the light water moderator which moderates quickly but with more loss than heavy water. Moreover, the PWR is the most common fission reactor in the world, and its technology is mastered for a long time.</p>
    </sec>
   </sec>
   <sec id="s3">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>3. Physical Model of the D-D Fusion Reactor</title>
    <sec id="s3_1">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>3.1. Introduction</title>
     <p>The physical model has been described in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>. One of the differences between the D-D reactor, as described in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>, and the D-D reactor used here is that the Beta factor is now limited to a realistic value. Consequently, the working conditions are very different. In <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>, it was possible to work with an equilibrium energy superior to 100 keV, the limit on Beta being equal to 0.5.</p>
     <p>With a realistic Beta, the equilibrium energy is now around 29 keV, so it is not much above the value for a Tokamak or a Stellarator, i.e., around 15 keV.</p>
     <p>Under these conditions, the mechanical gain Q for a Tokamak (ITER, for example) or a Stellarator (Helias project, for example) using D-T fusion, is expected to be equal or superior to 10. For a Stellarator using D-D fusion, the mechanical gain is expected to be widely inferior to 1, because the fusion reactivity of the D-D fusion is low compared to the D-T one (see <xref ref-type="fig" rid="fig5">
       Figure 5
      </xref>).</p>
    </sec>
    <sec id="s3_2">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>3.2. Beta Factor Considered</title>
     <p>It is reminded the Beta factor as determined in the Appendix A of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Beta 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            5.369 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mo>
            − 
          </mo> 
          <mn>
            25 
          </mn> 
          <mo>
            × 
          </mo> 
          <mtext>
            ne 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            E_equi 
          </mtext> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              eV 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             B 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (3.1)</p>
     <p>With E_equi, the equilibrium energy of the plasma in eV, ne the electron density (number of electrons per m<sup>3</sup>), and B the toroidal magnetic field (T) in the fusion reactor.</p>
     <p>The limit of Beta was 0.5 for the D-D reactor described in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>, which is not feasible for the present Stellarators, as the present actual limit is between 0.05 and 0.06 (<xref ref-type="bibr" rid="scirp.137109-15">
       [15]
      </xref>).</p>
     <p>So, we will consider this value of Beta = 0.05 as the default maximum value for the calculation of the D-D fusion reactor.</p>
     <p>Simulations with Beta = 0.06 and with Beta = 0.15, this last value being considered as a possible target for the future according to <xref ref-type="bibr" rid="scirp.137109-14">
       [14]
      </xref>, are also proposed by the “D_D_PWR_hybrid_reactor” program (§1.5).</p>
     <p>As said in <xref ref-type="bibr" rid="scirp.137109-14">
       [14]
      </xref>, if the improvement of the toroidal magnetic field seems difficult above the present values (5 or 6 T), the improvement of Beta above 0.05 seems promising. For example, from the default configuration, with Beta = 5%: Q = 0.184 and the average electric power is equal to 1437 MWe, whereas with Beta = 6%: Q = 0.215 (+17%) and the average electric power is equal to 2223 MWe (+55%). Moreover, with Beta = 6%, for the same electric power of 1437 MWe, the radius only needs to be equal to 178 cm instead of 200 cm, which gives -30% in terms of volume.</p>
     <p>Here is another example. With a maximum Beta equal to 0.15, the minimum size, for almost the same average net power (1381 MWe), is half of the size of the default configuration, i.e., a radius of Rp = 1 m instead of Rp = 2 m. Note that in these conditions, with a maximum K_eff = 0.94 instead of 0.9 (§4.5), the average net power would be about double (2779 MWe).</p>
    </sec>
    <sec id="s3_3">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>3.3. Energy Confinement Time Tct (s) in the Half-Toruses</title>
     <p>The equilibrium energy (29 keV, so T = 19 keV) is not so far away from the one of Helias Stellarators (15 keV maximum on <xref ref-type="bibr" rid="scirp.137109-11">
       [11]
      </xref> (p. 19), for example). So there is no need to apply special scaling formulas (for the half-toruses) to take into account a high equilibrium energy (i.e., &gt;100 keV): in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> §2.2.8, it was used the Kovrizhnikh (or the Bohm) scaling formula to estimate Tct.</p>
     <p>For the present Stellarators, it is in general, used the ISS04 scaling (<xref ref-type="bibr" rid="scirp.137109-15">
       [15]
      </xref> for example):</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Tct 
        </mtext> 
        <mo>
          = 
        </mo> 
        <msub> 
         <mi>
           f 
         </mi> 
         <mrow> 
          <mi>
            r 
          </mi> 
          <mi>
            e 
          </mi> 
          <mi>
            n 
          </mi> 
         </mrow> 
        </msub> 
        <mo>
          × 
        </mo> 
        <mn>
          0.134 
        </mn> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           a 
         </mi> 
         <mrow> 
          <mn>
            2.28 
          </mn> 
         </mrow> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mrow> 
          <mn>
            0.64 
          </mn> 
         </mrow> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           P 
         </mi> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            0.61 
          </mn> 
         </mrow> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mtext>
            ne 
          </mtext> 
         </mrow> 
         <mrow> 
          <mn>
            0.54 
          </mn> 
         </mrow> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           B 
         </mi> 
         <mrow> 
          <mn>
            0.84 
          </mn> 
         </mrow> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msubsup> 
         <mi>
           t 
         </mi> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mo>
            / 
          </mo> 
          <mn>
            3 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            0.41 
          </mn> 
         </mrow> 
        </msubsup> 
       </mrow> 
      </math> (3.2)</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
        <mtr> 
         <mtd> 
          <mi>
            P 
          </mi> 
          <mo>
            = 
          </mo> 
          <mtext>
            P_heating_power_MW 
          </mtext> 
         </mtd> 
        </mtr> 
        <mtr> 
         <mtd> 
          <mo>
            = 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              PlostReactor 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mtext>
              Pra 
            </mtext> 
            <mo>
              − 
            </mo> 
            <mtext>
              Pah 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mtext>
            Torus_volume_m 
          </mtext> 
          <mn>
            3 
          </mn> 
          <mo>
            / 
          </mo> 
          <mn>
            1 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            6 
          </mn> 
         </mtd> 
        </mtr> 
       </mtable> 
      </math> (3.3)</p>
     <p>with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Torus_volume_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mn>
          2 
        </mn> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          × 
        </mo> 
        <mi>
          r 
        </mi> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mtext>
            Rp 
          </mtext> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </math> (3.4)</p>
     <p>It is implicitly supposed in the P calculation that the heating is the same in the entire reactor.</p>
     <p>The problem with this formula (Equation 3.2) is its big uncertainty on the confinement renormalization factor. For example, according to <xref ref-type="bibr" rid="scirp.137109-16">
       [16]
      </xref>, f<sub>ren</sub> can be between 1.0 and 1.5.</p>
     <p>To avoid this renormalization factor, a better solution is given by <xref ref-type="bibr" rid="scirp.137109-17">
       [17]
      </xref> in the form of 2 formulas that apply to the Helias 5-B Stellarator (“Shearless” configuration), which constitutes the model of both half-toruses. An average of these 2 formulas will certainly give a better result than the ISS004 scaling. This average is, in practice, very close to the ISS04 result. These two formulas to average are (from <xref ref-type="bibr" rid="scirp.137109-17">
       [17]
      </xref>):</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Tct_s1 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            0.0554 
          </mn> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mn>
              2.17 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mn>
              0.64 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             P 
           </mi> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              0.62 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mtext>
              ne 
            </mtext> 
           </mrow> 
           <mrow> 
            <mn>
              0.74 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             B 
           </mi> 
           <mrow> 
            <mn>
              1.25 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msubsup> 
           <mi>
             t 
           </mi> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mo>
              / 
            </mo> 
            <mn>
              3 
            </mn> 
           </mrow> 
           <mrow> 
            <mn>
              0.30 
            </mn> 
           </mrow> 
          </msubsup> 
         </mrow> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mn>
            1.44 
          </mn> 
          <mo>
            × 
          </mo> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              2 
            </mn> 
            <mo>
              × 
            </mo> 
            <mi>
              R 
            </mi> 
            <mo>
              / 
            </mo> 
            <mn>
              1.8377 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (3.5)</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Tct_s2 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            0.0527 
          </mn> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             a 
           </mi> 
           <mrow> 
            <mn>
              2.15 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             R 
           </mi> 
           <mrow> 
            <mn>
              0.62 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             P 
           </mi> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              0.62 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mtext>
              ne 
            </mtext> 
           </mrow> 
           <mrow> 
            <mn>
              0.71 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mi>
             B 
           </mi> 
           <mrow> 
            <mn>
              1.20 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msubsup> 
           <mi>
             t 
           </mi> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mo>
              / 
            </mo> 
            <mn>
              3 
            </mn> 
           </mrow> 
           <mrow> 
            <mn>
              0.20 
            </mn> 
           </mrow> 
          </msubsup> 
         </mrow> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mn>
            1.24 
          </mn> 
          <mo>
            × 
          </mo> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              2 
            </mn> 
            <mo>
              × 
            </mo> 
            <mi>
              R 
            </mi> 
            <mo>
              / 
            </mo> 
            <mn>
              1.8377 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (3.6)</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Tct 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Tct_s 
          </mtext> 
          <mn>
            1 
          </mn> 
          <mo>
            + 
          </mo> 
          <mtext>
            Tct_s 
          </mtext> 
          <mn>
            2 
          </mn> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </math> (3.7)</p>
     <p>These formulas apply to both half-toruses because together, they form a torus.</p>
     <p>If applied to the straight pipes of the fusion reactor (see <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>), these formulas would give an infinite confinement time due to an infinite R, which is not physical. In fact, this particular confinement time (TDexpsp) and the time confinement for the whole reactor (TDexp) are estimated in Appendix A of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
    </sec>
    <sec id="s3_4">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>3.4. About Charge Exchanges between Ions and Gas Neutrals</title>
     <p>In <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> (§2.2.4), it was supposed to exist permanent losses by charge exchanges on neutrals. This behavior exists at the beginning of the operation but disappears progressively as the fusion reactor wall is not in contact with gas, so charge exchanges will not be considered. Consequently, the variables 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          γ 
        </mi> 
        <mtext>
          cep 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          γ 
        </mi> 
        <mtext>
          ceT 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          γ 
        </mi> 
        <mtext>
          ceHe3 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          γ 
        </mi> 
        <mtext>
          ceHe4 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          γ 
        </mi> 
        <mtext>
          ceD 
        </mtext> 
       </mrow> 
      </math> will be forced to 0.</p>
    </sec>
    <sec id="s3_5">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>3.5. Important Results of the Fusion Reactor Calculation</title>
     <p>It has been supposed to have an Rp radius equal to 2.0 m (default value). The main results of the fusion reactor calculation are the following:</p>
     <p>Experimentally, it appears that a good performance for a fission reactor supplied by a D-D fusion reactor occurs when the product “Q × PnDDm3”, used as a “quality” criterion, is maximum. Q is the mechanical gain and PnDDm3 the fusion power of 2.45 MeV neutrons. Now, this criterion is probably not the best one.</p>
     <p>The rate of fusion neutrons generated from the two straight lines per sec (Qns_2L) is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Qns_2L 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          V_straight_lines_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Qfnm 
        </mtext> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </math> (3.8)</p>
     <p>with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Qfnm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mtext>
          QfDDm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          2 
        </mn> 
        <mo>
          + 
        </mo> 
        <mtext>
          QfDTm 
        </mtext> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </math> (3.9)</p>
     <p>Qfnm3 is the rate of fusion neutrons (at 2.45 and 14.06 MeV) generated per s and per m<sup>3</sup>.</p>
     <p>For QfDDm3 and QfDTm3 refer to <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
     <p>with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          V_straight_lines_m3 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          60 
        </mn> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mtext>
            Rp 
          </mtext> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </math> (3.10)</p>
     <p>the global volume in m<sup>3</sup> of both straight lines.</p>
     <p>The consumed mechanical power, in W, for the whole fusion reactor (Pm_input_W) is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pm_input_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          V_fusion_reactor_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Pinput 
        </mtext> 
       </mrow> 
      </math> (3.11)</p>
     <p>with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          V_fusion_reactor_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mn>
          66 
        </mn> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mi>
           π 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mtext>
            Rp 
          </mtext> 
         </mrow> 
         <mn>
           3 
         </mn> 
        </msup> 
       </mrow> 
      </math> (3.12)</p>
     <p>For Pinput, refer to <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
     <p>The fusion power, in W, for the whole fusion reactor (Pth_fusion_W) is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          P 
        </mi> 
        <mtext>
          th_fusion_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          V_fusion_reactor_m3 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          Poutput 
        </mtext> 
       </mrow> 
      </math> (3.13)</p>
     <p>With 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Poutput 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pneu 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          PlostFi 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          PlostReactor 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Pra 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pfusion 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Pinput 
        </mtext> 
       </mrow> 
      </math> at equilibrium (Equations B11 and B12 of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>). For these variables, refer to <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>.</p>
     <p>The neutron power, generated by 2.45 and 14.06 MeV neutrons, issued from the volume of the straight lines of the fusion reactor, is equal to Equation 3.13 bis: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          P_neutron_2L_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            PfnDDm3 
          </mtext> 
          <mo>
            + 
          </mo> 
          <mtext>
            PfnDTm3 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          × 
        </mo> 
        <mtext>
          V_straight_lines_m3 
        </mtext> 
       </mrow> 
      </math>.</p>
     <p>With PfnDDm3+PfnDTm3 = Pneu (global neutronic power per m<sup>3</sup>, refer to <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> for details).</p>
     <p>The proportion of neutrons at 2.45 MeV among all the neutrons generated at 2.45 and 14.06 MeV is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pro_n_2_45_MeV 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            QfDDm 
          </mtext> 
          <mn>
            3 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mo>
            × 
          </mo> 
          <mtext>
            Qfnm 
          </mtext> 
          <mn>
            3 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (3.14)</p>
     <p>The surface heat power (SHP in W/m<sup>2</sup> §2.2.10 of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>) is now calculated for both half-toruses where the heat power is maximum and for the straight pipes where the heat power is minimum:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          SHPmax 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              PlostFi 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mtext>
              PlostHT 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mtext>
              Pra 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mtext>
            Rp 
          </mtext> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </math> (3.15)</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          SHPmin 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              PlostFi 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mtext>
              PlostD 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mtext>
              Pra 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mtext>
            Rp 
          </mtext> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </mfrac> 
       </mrow> 
      </math> (3.16)</p>
    </sec>
   </sec>
   <sec id="s4">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>4. Physical Model of the PWR Fission Reactor and the Water Steam Circuit</title>
    <sec id="s4_1">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.1. Introduction</title>
     <p>At this level, the fusion reactor has been calculated. The main parameters are known, i.e.:</p>
     <p>Rp_cm (Rp_cm = Rp x 100), Qns_2L, Pm_input_W, Pth_fusion_W and Pro_n_2_45_MeV.</p>
     <p>Now, the user proposes a mixture of U235, U238, and Th232 in terms of atomic concentrations, the total being equal to 1 (100%).</p>
     <p>First, the fission reactor dimensions, the mass of fuel, etc., will be calculated.</p>
     <p>Once the fission reactor is determined, the calculation will be incremental by step of one hour. It will be first calculated the reactivity, the thermal fission power generated, the net electric power and the evolution of the fuel. Results will be displayed per year. The main result is the average net electrical power.</p>
     <p>The number of years calculated is determined by the user, but by default, 100 years are proposed, 100 years being the minimum expected service life for this reactor (see §5.5).</p>
    </sec>
    <sec id="s4_2">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.2. First Wall</title>
     <p>The wall between the fusion reactor and the fission reactor must be a solid non-ferromagnetic metal able to support heat, such as Beryllium, Copper alloy, Austenitic stainless steel, etc. Now, the sole metal able to let cross fast neutrons with few neutron absorptions is the Beryllium.</p>
     <p>The estimation of the probability Pnc of non-collision of a 2.45 MeV neutron across a certain thickness of Beryllium is based on the method shown in <xref ref-type="bibr" rid="scirp.137109-18">
       [18]
      </xref> (p. 290), normally used for an infinite plate, so conservative here.</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pnc 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mstyle displaystyle="true"> 
           <mrow> 
            <munderover> 
             <mo>
               ∫ 
             </mo> 
             <mn>
               0 
             </mn> 
             <mrow> 
              <mi>
                π 
              </mi> 
              <mo>
                / 
              </mo> 
              <mn>
                2 
              </mn> 
             </mrow> 
            </munderover> 
            <mrow> 
             <mi>
               sin 
             </mi> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mi>
                θ 
              </mi> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               × 
             </mo> 
             <mi>
               cos 
             </mi> 
            </mrow> 
           </mrow> 
          </mstyle> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mi>
             θ 
           </mi> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mi>
              a 
            </mi> 
            <mo>
              × 
            </mo> 
            <mi>
              Σ 
            </mi> 
            <mi>
              t 
            </mi> 
            <mo>
              / 
            </mo> 
            <mi>
              cos 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mi>
               θ 
             </mi> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mtext>
            d 
          </mtext> 
          <mi>
            θ 
          </mi> 
         </mrow> 
         <mrow> 
          <mstyle displaystyle="true"> 
           <mrow> 
            <munderover> 
             <mo>
               ∫ 
             </mo> 
             <mn>
               0 
             </mn> 
             <mrow> 
              <mi>
                π 
              </mi> 
              <mo>
                / 
              </mo> 
              <mn>
                2 
              </mn> 
             </mrow> 
            </munderover> 
            <mrow> 
             <mi>
               sin 
             </mi> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mi>
                θ 
              </mi> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               × 
             </mo> 
             <mi>
               cos 
             </mi> 
            </mrow> 
           </mrow> 
          </mstyle> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mi>
             θ 
           </mi> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            × 
          </mo> 
          <mtext>
            d 
          </mtext> 
          <mi>
            θ 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math></p>
     <p>With Σt the collision macroscopic cross-section, a the beryllium thickness and θ the colatitude.</p>
     <p><u>Note</u>: the cross sections data of materials are taken from the library ENDF/B-VIII.0.</p>
     <p>From Pnc and knowing the diffusion and the absorption cross sections at different energies, it can be calculated (with a small program) the average probability that a neutron crosses the wall and the average energy just after the crossing. For a Beryllium thickness of 5 cm, the probability for a 2.45 MeV neutron to cross the wall is equal to 0.915, with a final average energy of 1.12 MeV. This thickness of 5 cm is considered the best compromise between resistance and neutron transparency and will be selected for the following.</p>
     <p>For about the 14.06 MeV neutrons, it must be taken into account the n-2n reaction:</p>
     <p>n + <sup>9</sup>Be ◊2n + 2 <sup>4</sup>He − 1.57 MeV</p>
     <p>After a calculation similar to the previous one, it can be determined that for a Beryllium thickness of 5 cm, 2.9% of these neutrons are lost before reaching the energy of 2.45 MeV and, for the rest, the amplification factor is equal to 1.478. So the global probability PTr_Br for a neutron (initial or created via the n-2n reaction) to cross the 5 cm Beryllium wall is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Ptr_Be 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          0.915 
        </mn> 
        <mo>
          × 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            Pro_n_2_45_MeV 
          </mtext> 
          <mo>
            + 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              Pro_n_14_06_MeV 
            </mtext> 
            <mo>
              × 
            </mo> 
            <mn>
              0.971 
            </mn> 
            <mo>
              × 
            </mo> 
            <mn>
              1.478 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </math>(4.1)</p>
     <p>With 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pro_n_14_06_MeV 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          1 
        </mn> 
        <mo>
          − 
        </mo> 
        <mtext>
          Pro_n_2_45_MeV 
        </mtext> 
       </mrow> 
      </math> (4.2)</p>
    </sec>
    <sec id="s4_3">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.3. Temperature and Pressure Conditions of the Main Fission Primary System</title>
     <p>According to <xref ref-type="bibr" rid="scirp.137109-19">
       [19]
      </xref>, the minimum elastic limit of Beryllium is equal to 170 MPa (1700 bar), for a maximum of 575 MPa. The average elastic limit is equal to 372.5 Mpa, and an elastic limit of 280 Mpa will be chosen.</p>
     <p><u>Note</u>: it is supposed that the first wall in Beryllium and the exterior wall in 316LN are united by a fine structure to strengthen the first wall against buckling and, hence, to avoid considering an elastic limit that is too low.</p>
     <p>So, the maximum pressure on the main primary system in bar abs (Pfr_bar_abs) to avoid the bucking can be estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pfr_bar_abs 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            a_Be_cm 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            Elastic limit 
          </mtext> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              bar 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mtext>
            Rp_cm 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            5 
          </mn> 
          <mo>
            × 
          </mo> 
          <mn>
            2800 
          </mn> 
         </mrow> 
         <mrow> 
          <mtext>
            Rp_cm 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            14000 
          </mn> 
         </mrow> 
         <mrow> 
          <mtext>
            Rp_cm 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.3)</p>
     <p>The saturation temperature (Tsat_C), for a pressure between 20 and 155 bar abs, can be estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          T_sat_C 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          100 
        </mtext> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mtext>
            Pfr_bar_abs 
          </mtext> 
         </mrow> 
         <mi>
           X 
         </mi> 
        </msup> 
       </mrow> 
      </math> (4.4)</p>
     <p>with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
        <mtr> 
         <mtd> 
          <mi>
            X 
          </mi> 
          <mo>
            = 
          </mo> 
          <mn>
            0.249755 
          </mn> 
          <mo>
            × 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <mn>
              0.017357 
            </mn> 
            <mo>
              × 
            </mo> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mtext>
                  Pfr_bar_abs 
                </mtext> 
                <mo>
                  − 
                </mo> 
                <mn>
                  30 
                </mn> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
             </mrow> 
            </mrow> 
           </mrow> 
          </mrow> 
         </mtd> 
        </mtr> 
        <mtr> 
         <mtd> 
          <mtext>
              
          </mtext> 
          <mtext>
              
          </mtext> 
          <mtext>
              
          </mtext> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mtext>
               Sign 
             </mtext> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mtext>
                 Pfr_bar_abs 
               </mtext> 
               <mo>
                 − 
               </mo> 
               <mn>
                 30 
               </mn> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mn>
               124 
             </mn> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
           <mrow> 
            <mn>
              0.5 
            </mn> 
           </mrow> 
          </msup> 
          <mo>
            × 
          </mo> 
          <mrow> 
           <mrow> 
            <mtext>
              Sign 
            </mtext> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mtext>
                Pfr_bar_abs 
              </mtext> 
              <mo>
                − 
              </mo> 
              <mn>
                30 
              </mn> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mtd> 
        </mtr> 
       </mtable> 
      </math> and Sign(Pfr_bar_abs-30) = 1 if Pfr_bar_abs ≥ 30, and Sign(Pfr_bar_abs-30) = −1 reversely.</p>
     <p>The water inside the main primary system pressurizer being at T_sat_C and the difference between the pressurizer temperature and the primary temperature at 100% of the nominal power (Tfr_C) being supposed equal to 30˚C, it can be deduced:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Tfr_C 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          T_sat_C 
        </mtext> 
        <mo>
          − 
        </mo> 
        <mn>
          30 
        </mn> 
       </mrow> 
      </math> (4.5)</p>
     <p>Note that for the default value Rp_cm = 200 cm, the pressure is equal to 70 bar abs and the primary temperature is equal to 256˚C, i.e., much less that the standard conditions of an EPR (155 bar abs and 313˚C).</p>
    </sec>
    <sec id="s4_4">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.4. Gross Electrical Yield (Yg) and Gross Power Delivered by the Alternator (Pe_gross_W)</title>
     <p>In what follows, it is considered a thermodynamic conversion of the output power in the form of heat (Psg_W) supplied by the fission reactor in electricity (see <xref ref-type="fig" rid="fig4">
       Figure 4
      </xref>). The reference gross yield Yg = 0.39 of this conversion corresponds to the gross yield of a modern fission reactor, as the EPR one.</p>
     <p>Let’s suppose that for an EPR, this Yg value is obtained for an average main primary temperature (Tfr_C) of 312.9˚C and a heat sink temperature of 34˚C. The theoretical Carnot yield would be equal to 0.4789. So, the EPR yield compared to the Carnot yield is equal to 0.82. Now, let’s suppose that Yg is always proportional to the Carnot yield and to the EPR yield compared to the Carnot yield. It can be deduced the probable Yg for a given Tfr_C:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Yg 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Tfr_C 
          </mtext> 
          <mo>
            − 
          </mo> 
          <mn>
            34 
          </mn> 
         </mrow> 
         <mrow> 
          <mtext>
            Tfr_C 
          </mtext> 
          <mo>
            + 
          </mo> 
          <mn>
            273.15 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mn>
          0.82 
        </mn> 
       </mrow> 
      </math> (4.6)</p>
     <p>So the gross power delivered by the alternator will be equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_gross_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Yg 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          Psg_W 
        </mtext> 
       </mrow> 
      </math> (4.7)</p>
     <p>With Psg_W calculated in §2.1.</p>
    </sec>
    <sec id="s4_5">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.5. Preliminary Calculations Relative to the Fission Reactor</title>
     <p>The model of PWR used for calculations of this reactor about reactivity, thermal power, geometric values, etc, is the P4/P’4 1300 MWe one developed in France by EDF + Framatome and based on a Westinghouse model (South Texas). This P4/P’4 model is chosen because a proposal for the complete calculation of this type of reactor is given in <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref>. This calculation based on Uranium only has been extended, in this paper, to Plutonium, Thorium and minor actinides.</p>
     <p><u>Note 1</u>: the necessary data as ν (“Nu”), the average number of neutrons emitted by thermal fissions, the energy generated by fission, the thermal cross-sections, the specific gravities, the resonance integrals, the atomic masses, the number of atoms per cm<sup>3</sup>, etc are extracted from <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>.</p>
     <p><u>Note 2</u>: it is supposed that the working of a PWR is known, as it will not be detailed. For example, see <xref ref-type="bibr" rid="scirp.137109-22">
       [22]
      </xref> for an abstract about PWR.</p>
     <p><u>Note 3</u>: the calculations given in <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref> and conventional calculations will not be (re)presented in the rest of this document, but will be present in the source code of the “D_D_PWR_hybrid_reactor” program, if relevant. However, other calculations will be described below. Note that for neutronic calculations, nuclear research centers and engineering companies use powerful programs (see <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>).</p>
     <p><u>About the maximum</u> <u>reactivity allowed</u></p>
     <p>The reactor being sub-critical, there is no need for the full-length rod control system. The negative reactivity weight of all these rods for a P4/P’4 reactor is, at maximum, a bit below 11,000 pht (“pht” for “Per hundred thousand”, i.e., in 1/100,000). So it will be considered that the reactor (normally critical) must work here, at best, at an effective multiplication factor (K_eff) corresponding to all rods inserted, so 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          K_eff 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              11000 
            </mn> 
            <mo>
              / 
            </mo> 
            <mn>
              1 
            </mn> 
            <mtext>
              E 
            </mtext> 
            <mn>
              5 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mn>
          0.9 
        </mn> 
       </mrow> 
      </math>. For a real K_eff &gt; 0.9, the reactor water must be borated, so as to remain at K_eff = 0.9. Reversely, for a real K_eff ≤ 0.9, the water must be the least borated possible. This value of 0.9 will be commonly reached, so the water will be, in general, borated.</p>
     <p>This maximum of 0.9 will be used to calculate the fission reactor.</p>
     <p><u>Note</u>: <u>this hypothesis is important</u>. For example, for a maximum K_eff = 0.95 instead of 0.9, the average net electrical power is about 2.5 larger, as for example, for the default configuration: 3669 MWe instead of 1437 MWe. However, with a maximum K_eff = 0.95 instead of 0.9, the core meltdown probability will be a bit larger even if still extremely low (see §5.9).</p>
     <p>The number of fuel (U_Th_02) atoms per cm<sup>3</sup> of this fission reactor (N_fuel) is estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable> 
        <mtr> 
         <mtd> 
          <mtext>
            N_fuel 
          </mtext> 
          <mo>
            = 
          </mo> 
          <mfrac> 
           <mrow> 
            <mtext>
              Mean_fuel_specific_gravity 
            </mtext> 
            <mo>
              × 
            </mo> 
            <mtext>
              Avogadro_number 
            </mtext> 
            <mo>
              × 
            </mo> 
            <mn>
              0.281695 
            </mn> 
           </mrow> 
           <mrow> 
            <mtext>
              A_fuel 
            </mtext> 
           </mrow> 
          </mfrac> 
         </mtd> 
        </mtr> 
        <mtr> 
         <mtd> 
          <mtext>
              
          </mtext> 
          <mtext>
              
          </mtext> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mo>
              ( 
            </mo> 
            <mrow> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mrow> 
               <mtext>
                 Tfr_C 
               </mtext> 
               <mo>
                 + 
               </mo> 
               <mn>
                 273.15 
               </mn> 
              </mrow> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               / 
             </mo> 
             <mn>
               293.15 
             </mn> 
            </mrow> 
            <mo>
              ) 
            </mo> 
           </mrow> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              0.023592 
            </mn> 
           </mrow> 
          </msup> 
         </mtd> 
        </mtr> 
       </mtable> 
      </math> (4.8)</p>
     <p>With A_fuel the atomic mass in g of the fuel, mixture of U235, U238, Th232 and O2 (i.e., U02+TH02).</p>
     <p>The molar moderating ratio (MR) is estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          MR 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            3.88553 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            22 
          </mn> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mrow> 
               <mo>
                 ( 
               </mo> 
               <mrow> 
                <mtext>
                  Tfr_C 
                </mtext> 
                <mo>
                  + 
                </mo> 
                <mn>
                  273.15 
                </mn> 
               </mrow> 
               <mo>
                 ) 
               </mo> 
              </mrow> 
              <mo>
                / 
              </mo> 
              <mn>
                293.15 
              </mn> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mn>
              0.42173 
            </mn> 
           </mrow> 
          </msup> 
         </mrow> 
         <mrow> 
          <mtext>
            N_fuel 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.9)</p>
    </sec>
    <sec id="s4_6">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.6. Maximum Power Produced by Fission According to the Fusion Neutrons Flux, for K_eff = 0.9</title>
     <p>The neutrons flux (Qns_2L) issued from the straight parts of the fusion reactor and having crossed the Beryllium wall is multiplied by a factor equal to 1/(1-K_eff), cf. <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref> (p. 86).</p>
     <p>The maximum effective multiplication factor K_eff = 0.9 is used to size the fission reactor.</p>
     <p>So 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Qn_fr 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Qns_2L 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            Ptr_Be 
          </mtext> 
         </mrow> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.10)</p>
     <p>with Ptr_Be defined in §4.2</p>
     <p>The probability for a neutron to generate a fission is equal to 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          w 
        </mi> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Mean_Nu 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> Mean_Nu, the average number of neutrons emitted by thermal fission, depends on the fuel.</p>
     <p>So the number of fissions par sec is equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Qf_fr 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Qn_fr 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Mean_Nu 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.11)</p>
     <p>The maximum thermal power generated by fissions in the reactor (Pth_fission_MW) is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
        <mtr> 
         <mtd> 
          <mtext>
            Pth_fission_MW 
          </mtext> 
         </mtd> 
        </mtr> 
        <mtr> 
         <mtd> 
          <mo>
            = 
          </mo> 
          <mtext>
            Qf_fr 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            Mean_energy_release_per_fission_MeV 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mn>
            1.60219 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mo>
            − 
          </mo> 
          <mn>
            19 
          </mn> 
         </mtd> 
        </mtr> 
       </mtable> 
      </math> (4.12)</p>
     <p>with Mean_energy_release_per_fission_MeV, which depends on the fuel.</p>
    </sec>
    <sec id="s4_7">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.7. Dimension of the Fusion Reactor, for K_eff = 0.9</title>
     <p>The interior radius of the fission reactor is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Ri_fr_cm 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Rp_cm 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Beryllium_thickness_cm 
        </mtext> 
       </mrow> 
      </math> (4.13)</p>
     <p>The minimum volume of the core (fuel assemblies), on the basis of a P4/P’4 reactor (i.e., 99.64 MW/m<sup>3</sup> at 20˚C, cf. <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref>) at 20˚C and at Tfr_C is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Vco_m3_at_20_C 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Pth_fission_MW 
          </mtext> 
         </mrow> 
         <mrow> 
          <mn>
            99.64 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.14)</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Vco_m3_at_Tfr 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Vco_m3_at_20_C 
        </mtext> 
        <mo>
          × 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mtext>
                Tfr_C 
              </mtext> 
              <mo>
                + 
              </mo> 
              <mn>
                273.15 
              </mn> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
            <mo>
              / 
            </mo> 
            <mn>
              293.15 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mn>
            0.023592 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
      </math> (4.15)</p>
     <p>The exterior radius of the core is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Re_co_cm_at_Tfr 
        </mtext> 
        <mo>
          = 
        </mo> 
        <msqrt> 
         <mrow> 
          <msup> 
           <mrow> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mtext>
                Ri_fr_cm 
              </mtext> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            + 
          </mo> 
          <mfrac> 
           <mrow> 
            <mtext>
              Vco_m3_at_Tfr 
            </mtext> 
            <mo>
              × 
            </mo> 
            <mn>
              1 
            </mn> 
            <mtext>
              E 
            </mtext> 
            <mn>
              6 
            </mn> 
           </mrow> 
           <mrow> 
            <mn>
              2 
            </mn> 
            <mo>
              × 
            </mo> 
            <mi>
              π 
            </mi> 
            <mo>
              × 
            </mo> 
            <mtext>
              L_cm 
            </mtext> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </math> (4.16)</p>
     <p>The thickness of the core is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          THco_cm_at_Tfr 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Re_co_cm_at_Tfr 
        </mtext> 
        <mo>
          − 
        </mo> 
        <mtext>
          Ri_fr_cm 
        </mtext> 
       </mrow> 
      </math> (4.17)</p>
     <p>It is reminded that the core of the fission reactor is composed of a certain number of fuel assemblies. Each fuel assembly is composed of long fuel rods separated by water. For this reactor, it is implicitly supposed that the fuel assemblies are the ones used on P4/P’4 plants for the reactivity calculation. However, the fuel assemblies will necessarily be modified as the rods will be longer and the fuel assembly will have a smaller section.</p>
     <p>Note that for a P4/P’4 fuel assembly, there are 264 fuel rods for 289 passages. The remaining 25 passages are used for control rods, burnable poison, neutron sources and instrumentation in the central passage. Only the central passage for instrumentation would be useful for this type of hybrid reactor. The remaining 24 passages could be used for fuel rods, which would increase the reactivity without affecting the compactness.</p>
     <p>Otherwise, it has been estimated, for reasons relative to the minimum displacement of neutrons on the reactor and to the leakage of the reactor, that the core thickness (THco_cm_at_Tfr) must not be inferior to 12 cm.</p>
     <p>So, if the thickness result is inferior to 12 cm, it will be switched to 12 cm and the parameters Re_co_cm, Vco_m3_at_20C, and Vco_m3_at_Tfr will be re-calculated using the reverse equations of the equations 4.14 to 4.16.</p>
     <p>The reflector (light water) surrounds the fuel assemblies. Its thickness is supposed to be equal to 20 cm (estimated average value for a PWR). So, the thickness reflector saving is equal to 8.27 cm, according to <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref>. Note that relatively to thermal neutrons, the Beryllium wall is considered transparent.</p>
     <p>The interior radius of the exterior wall in 316LN is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Ri_ew_cm 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Re_co_cm 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Reflector_thickness_cm 
        </mtext> 
       </mrow> 
      </math> (4.18)</p>
     <p>To bear the primary pressure (Pfr_bar_gauge), the thickness of the exterior wall in 316LN is estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          TH_ew_cm 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Pfr_bar_gauge 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            Ri_ew_cm 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Minimum elastic limit for 316LN 
          </mtext> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              bar 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            − 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              Pfr_bar_gauge 
            </mtext> 
            <mo>
              / 
            </mo> 
            <mn>
              2 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math>(4.19)</p>
     <p>With 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pfr_bar_gauge 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pfr_bar_abs 
        </mtext> 
        <mo>
          − 
        </mo> 
        <mn>
          1 
        </mn> 
       </mrow> 
      </math> (4.20)</p>
     <p>The minimum elastic limit for 316LN is considered equal to 100 Mpa for a nominal value of 205 MPa (<xref ref-type="bibr" rid="scirp.137109-23">
       [23]
      </xref>).</p>
     <p>TH_ew_cm is equal to 16.9 cm for the default configuration.</p>
     <p>The exterior radius of the exterior wall in 316LN is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Re_ew_cm 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Ri_ew_cm 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          TH_ew_cm 
        </mtext> 
       </mrow> 
      </math> (4.21)</p>
     <p>Note that this exterior radius is the interior radius of the system supporting the magnetic coils cooled by the cryogenic fluid (see <xref ref-type="bibr" rid="scirp.137109-11">
       [11]
      </xref>).</p>
    </sec>
    <sec id="s4_8">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.8. Determination of the Net and Auxiliary Power Delivered by the Alternator</title>
     <p>Several consumers must be supplied with electricity by the alternator before supplying the first useful watt (see <xref ref-type="fig" rid="fig4">
       Figure 4
      </xref>). They are quantified below.</p>
     <p>The cryogenic system necessary to cool the superconducting coils is proportional to the area covered by the coils. From the Helias data, it has been determined that the specific electrical power for cryogenics (mainly used by magnetic coils) is about 13600 W/m<sup>2</sup>.</p>
     <p>The circumference in m of the fusion reactor (at the axis) is equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Cfr_m 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          66 
        </mn> 
        <mo>
          × 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          × 
        </mo> 
        <mtext>
          Rp_cm 
        </mtext> 
        <mo>
          / 
        </mo> 
        <mn>
          100 
        </mn> 
       </mrow> 
      </math> (4.22)</p>
     <p>So, the necessary cryogenic power for superconducting coils is estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_cryogenic_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Cfr_m 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mn>
          2 
        </mn> 
        <mo>
          × 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          × 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            Re_ew_cm 
          </mtext> 
          <mo>
            / 
          </mo> 
          <mn>
            100 
          </mn> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          × 
        </mo> 
        <mn>
          13600 
        </mn> 
       </mrow> 
      </math> (4.23)</p>
     <p>For UHV (Ultra High Vacuum) needs, it will be supposed that the electrical consumption is equal to 20% of the cryogenic power for superconducting coils, so</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_UHV_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pe_cryogenic_W 
        </mtext> 
        <mo>
          / 
        </mo> 
        <mn>
          5 
        </mn> 
       </mrow> 
      </math> (4.24)</p>
     <p>As it is supposed that the efficiency of the D+ ions/electrons injectors of the fusion reactor is equal to 0.8, the electrical power consumed is equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_input_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pm_input_W 
        </mtext> 
        <mo>
          / 
        </mo> 
        <mn>
          0.8 
        </mn> 
       </mrow> 
      </math> (4.25)</p>
     <p>These 3 consumptions are fixed. The total is equal to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_fixed_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pe_cryogenic_W 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Pe_UHV_W 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mtext>
          Pe_input_W 
        </mtext> 
       </mrow> 
      </math> (4.26)</p>
     <p>Moreover, the plant needs electrical power for auxiliary equipment (pumps, valves, instrumentation, control…). It will be considered that it is equal to a fraction of the thermal power delivered to the steam generators. Based on the P4/P’4 plants:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_aux_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          0.0131 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Psg_W 
        </mtext> 
       </mrow> 
      </math> (4.27)</p>
     <p>With Psg_W calculated in §2.1.</p>
     <p>So the net power delivered by the alternator to the grid is equal to:</p>
     <p>
      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pe_net_W 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pe_gross_W 
        </mtext> 
        <mo>
          − 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            Pe_fixed_W 
          </mtext> 
          <mo>
            + 
          </mo> 
          <mtext>
            Pe_aux_W 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </math> (4.28)</p>
     <p><u>Note</u>: Pe_gross_W is always positive, while Pe_net_W can be:</p>
     <p>From Pe_net_W, the average electrical net power over the whole working of the reactor (Pe_average_MW) is calculated.</p>
    </sec>
    <sec id="s4_9">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.9. Determination of the Multiplication Factors: Infinite (K_Infinite) and Effective (K_eff)</title>
     <p>For information about K_infinite, K_eff and the non-leakage probability, see <xref ref-type="bibr" rid="scirp.137109-24">
       [24]
      </xref> or <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref> (pp. 115, 155).</p>
     <p>The infinite multiplication factor K_infinite is calculated according to <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref>. The calculation of <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref> is done in hot standby (critical) for enriched U235/U238 fresh fuel. It will be carried to the “full power” reactor state and extended to a fuel containing Uranium, Plutonium, Thorium, minor actinides, and fission products.</p>
     <p>About the K_infinite factor, below is reminded of the method. It is calculated supposing a reactor of infinite dimensions. 
      <math xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          K_infinite 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          η 
        </mi> 
        <mo>
          × 
        </mo> 
        <mi>
          f 
        </mi> 
        <mo>
          × 
        </mo> 
        <mi>
          p 
        </mi> 
        <mo>
          × 
        </mo> 
        <mi>
          ε 
        </mi> 
       </mrow> 
      </math> with:</p>
     <p>The reactor has finite dimensions, so it is necessary to estimate the non-leakage probability of fast and thermal neutrons (Pnl). It is taken into account by K_eff, according to <xref ref-type="bibr" rid="scirp.137109-25">
       [25]
      </xref> (p. 80).</p>
     <p><u>Note</u>: for the neutrons issued from the core and crossing the Beryllium wall (so without being reflected), this wall and the interior fusion reactor are considered transparent. The leakage in only considered towards the exterior.</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          K_eff 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          K_infinite 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          Pnl 
        </mtext> 
       </mrow> 
      </math> (4.29)</p>
     <p>and 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pnl 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <msup> 
             <mrow> 
              <mtext>
                Bg 
              </mtext> 
             </mrow> 
             <mn>
               2 
             </mn> 
            </msup> 
            <mo>
              × 
            </mo> 
            <mtext>
              Tau 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <msup> 
           <mrow> 
            <mtext>
              Lth 
            </mtext> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            × 
          </mo> 
          <msup> 
           <mrow> 
            <mtext>
              Bg 
            </mtext> 
           </mrow> 
           <mn>
             2 
           </mn> 
          </msup> 
          <mo>
            + 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.30)</p>
     <p>The slowing-down area Tau (also called “Fermi age”) for a PWR is equal to 50 (from <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 409).</p>
     <p>The diffusion area of thermal neutrons Lth<sup>2 </sup>for a PWR is equal to 6 (from <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 409).</p>
     <p>The geometric buckling Bg<sup>2</sup> is calculated for a cylinder of radius R (cm) and height H (cm) by (from <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 155):</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <msup> 
         <mrow> 
          <mtext>
            Bg 
          </mtext> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             j 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             R 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mfrac> 
         <mrow> 
          <msup> 
           <mi>
             π 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
         <mrow> 
          <msup> 
           <mi>
             H 
           </mi> 
           <mn>
             2 
           </mn> 
          </msup> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.31)</p>
     <p>with j = 2.40483</p>
     <p>Here H = L_cm with L_cm the straight pipe length equal to 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          L_cm 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          100 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          L_m 
        </mtext> 
       </mrow> 
      </math> and 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          L_m 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          30 
        </mn> 
        <mo>
          × 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          × 
        </mo> 
        <mtext>
          Rp 
        </mtext> 
       </mrow> 
      </math>(from <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>) (equation 4.31 bis)</p>
     <p>R is the exterior core radius added to the thickness reflector saving (8.27 cm, cf. §4.7), so here: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          R 
        </mi> 
        <mo>
          = 
        </mo> 
        <mtext>
          Re_co_cm_at_Tfr 
        </mtext> 
        <mo>
          + 
        </mo> 
        <mn>
          8.27 
        </mn> 
       </mrow> 
      </math></p>
     <p>Now the core is not a cylinder but a ring of interior radius Ri_fr_cm (cf. §4.7). So it will be supposed that: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <msup> 
         <mi>
           R 
         </mi> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          = 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              Re_co_cm_at_Tfr 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mn>
              8.27 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
        <mo>
          − 
        </mo> 
        <msup> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              Ri_fr_cm 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mn>
           2 
         </mn> 
        </msup> 
       </mrow> 
      </math></p>
     <p>The initial K_eff factor of <xref ref-type="bibr" rid="scirp.137109-20">
       [20]
      </xref> is calculated in hot standby, i.e., in a critical state, very close to 0% of the nominal power, the reactor temperature being close to the reactor nominal temperature at full power. The variation of the average moderator temperature between hot standby and full power, which depends on a temperature program, will be neglected relative to the reactivity and consequently to K_eff.</p>
     <p>However, increasing the nuclear power until the nominal power (100%) will introduce negative reactivity due to the Doppler effect on the fuel. Based on the Candu reactor data in <xref ref-type="bibr" rid="scirp.137109-26">
       [26]
      </xref>, it can be estimated that:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Doppler_pht 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Min 
        </mtext> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            400 
          </mn> 
          <mo>
            , 
          </mo> 
          <mn>
            850 
          </mn> 
          <mo>
            − 
          </mo> 
          <mn>
            450 
          </mn> 
          <mo>
            × 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              en_Pu 
            </mtext> 
            <mn>
              239 
            </mn> 
            <mo>
              + 
            </mo> 
            <mtext>
              en_Pu 
            </mtext> 
            <mn>
              241 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            / 
          </mo> 
          <mn>
            0.0026 
          </mn> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </math> (4.32)</p>
     <p>With en_Pu239 and en_Pu_241, the atomic concentrations of Pu239 and Pu241</p>
     <p>Again, from the Candu reactor data <xref ref-type="bibr" rid="scirp.137109-26">
       [26]
      </xref>, the negative reactivity introduced by Xenon and Samarium to reach the full power, from 0% of power, is estimated to 3350 pht.</p>
     <p>Still from the Candu reactor data <xref ref-type="bibr" rid="scirp.137109-26">
       [26]
      </xref>, the negative reactivity introduced by fission products between two refueling operations is estimated to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          nr_fp_pht 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          0.115 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Burnup_MWd_t 
        </mtext> 
       </mrow> 
      </math> (4.33)</p>
     <p>For the fuel burn-up, see §4.11.</p>
     <p>The total negative reactivity (in absolute) Negative_reactivity_pht is equal to the sum of these previous terms (Doppler effect, Xe + Sm and fission products).</p>
     <p>The initial reactivity at hot standby, in pht, is equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          ρ 
        </mi> 
        <mtext>
          _hs_pth 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            5 
          </mn> 
          <mo>
            × 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mi>
              K 
            </mi> 
            <mtext>
              _eff 
            </mtext> 
            <mo>
              − 
            </mo> 
            <mn>
              1 
            </mn> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math>(cf. <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 119) (4.34)</p>
     <p>It is negative because the reactor is in a sub-critical state.</p>
     <p>With the calculated absolute negative reactivity, the reactivity at full power moves to:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          ρ 
        </mi> 
        <mtext>
          _fp_pht 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mi>
          ρ 
        </mi> 
        <mtext>
          _hs_pht 
        </mtext> 
        <mo>
          − 
        </mo> 
        <mtext>
          Negative_reactivity_pht 
        </mtext> 
       </mrow> 
      </math> (4.35)</p>
     <p>So, at full power</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          K_eff 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mtext>
            ρ_fp_pht 
          </mtext> 
          <mo>
            / 
          </mo> 
          <mn>
            1 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            5 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.36)</p>
    </sec>
    <sec id="s4_10">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.10. Determination of the Thermal Neutrons Flux</title>
     <p>To simplify, the thermal neutrons flux (in neutrons/(cm<sup>2</sup> × s)) is the sole considered. The epithermal and the fast neutrons flux are not considered.</p>
     <p><u>Neutrons flux due to the sole fusion neutrons</u></p>
     <p>In the absence of reactivity, i.e., for a 100% natural Thorium fuel, the sole neutrons flux is the one generated by the fusion reactor. So, a minimum average neutrons flux across the core of the fission reactor must be calculated.</p>
     <p>The total neutrons flowrate generated by the fusion reactor is known: Qns_2L (calculated in §3.5).</p>
     <p>The source area (considered at the exterior of the Beryllium wall) is equal to</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Source_Area_cm2 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mn>
          2 
        </mn> 
        <mo>
          × 
        </mo> 
        <mi>
          π 
        </mi> 
        <mo>
          × 
        </mo> 
        <mtext>
          Ri_fr_cm 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mo>
            × 
          </mo> 
          <mtext>
            L_cm 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </math> (4.37)</p>
     <p>With Ri_fr_cm calculated in §4.7 and L_cm in §4.9.</p>
     <p>The flowrate of neutrons through this area is equal to 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          S_n_per_cm2_s 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Qns_2L 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mtext>
            Ptr_Be 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Source_Area_cm2 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math>.</p>
     <p>Ptr_Be, the probability for a neutron to cross the Beryllium wall, is defined in §4.2.</p>
     <p>To simplify, let’s consider that the neutron source is a plane surface.</p>
     <p>Moreover, it will be supposed that neutrons are thermal ones, which is simpler to manage but conservative as initial fast neutron displacement is much longer than the one of thermal neutrons. So, the neutrons issued from the Beryllium wall are considered to be slowed down immediately to thermal neutrons.</p>
     <p>The neutrons flux can be calculated using the formula from <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref> (p. 141): 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Flux 
        </mtext> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mi>
           x 
         </mi> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mtext>
          S_n_per_cm2_s 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mi>
            exp 
          </mi> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mo>
              − 
            </mo> 
            <mi>
              K 
            </mi> 
            <mo>
              × 
            </mo> 
            <mi>
              x 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mo>
            × 
          </mo> 
          <mi>
            K 
          </mi> 
          <mo>
            × 
          </mo> 
          <mi>
            D 
          </mi> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math>.</p>
     <p>With x the distance between the point considered inside the core and the exterior Beryllium surface (in cm).</p>
     <p>According to <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref> (pp. 142, 144), 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          K 
        </mi> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mtext>
            Lth 
          </mtext> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mtext>
              cm 
            </mtext> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <msqrt> 
           <mn>
             6 
           </mn> 
          </msqrt> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mn>
          0.408 
        </mn> 
        <mtext>
            
        </mtext> 
        <msup> 
         <mrow> 
          <mtext>
            cm 
          </mtext> 
         </mrow> 
         <mrow> 
          <mo>
            − 
          </mo> 
          <mn>
            1 
          </mn> 
         </mrow> 
        </msup> 
       </mrow> 
      </math> with Lth<sup>2</sup> defined in §4.9.</p>
     <p>D the diffusion coefficient is equal to 0.2 cm (<xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 144) for thermal neutrons.</p>
     <p>The average flux across the core thickness (THco_cm_at_Tfr, as defined in §4.7) is calculated this way:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Thermal_fusion_neutron_flux 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mstyle displaystyle="true"> 
           <mrow> 
            <munderover> 
             <mo>
               ∫ 
             </mo> 
             <mn>
               0 
             </mn> 
             <mrow> 
              <mtext>
                THfr_cm_at_Tfr 
              </mtext> 
             </mrow> 
            </munderover> 
            <mrow> 
             <mtext>
               Flux 
             </mtext> 
             <mrow> 
              <mo>
                ( 
              </mo> 
              <mi>
                x 
              </mi> 
              <mo>
                ) 
              </mo> 
             </mrow> 
             <mo>
               × 
             </mo> 
             <mtext>
               d 
             </mtext> 
             <mi>
               x 
             </mi> 
            </mrow> 
           </mrow> 
          </mstyle> 
         </mrow> 
         <mrow> 
          <mtext>
            THco_cm_at_Tfr 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math>,</p>
     <p>and after some developments:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mtable columnalign="left"> 
        <mtr> 
         <mtd> 
          <mtext>
            Thermal_fusion_neutron_flux 
          </mtext> 
         </mtd> 
        </mtr> 
        <mtr> 
         <mtd> 
          <mo>
            = 
          </mo> 
          <mfrac> 
           <mrow> 
            <mn>
              15 
            </mn> 
            <mo>
              × 
            </mo> 
            <mtext>
              S_n_per_cm2_s 
            </mtext> 
           </mrow> 
           <mrow> 
            <mtext>
              THco_cm_at_Tfr 
            </mtext> 
           </mrow> 
          </mfrac> 
          <mo>
            × 
          </mo> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              − 
            </mo> 
            <mi>
              exp 
            </mi> 
            <mrow> 
             <mo>
               ( 
             </mo> 
             <mrow> 
              <mo>
                − 
              </mo> 
              <mn>
                0.408 
              </mn> 
              <mo>
                × 
              </mo> 
              <mtext>
                THco_cm_at_Tfr 
              </mtext> 
             </mrow> 
             <mo>
               ) 
             </mo> 
            </mrow> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
         </mtd> 
        </mtr> 
       </mtable> 
      </math> (4.38)</p>
     <p><u>Normal average neutrons flux due to fusion + fission neutrons</u></p>
     <p>With reactivity (standard behavior), the neutron flux is determined this way.</p>
     <p>Let’s calculate the fission rate in neutrons per cm<sup>3</sup> and s:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Fission rate 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Qf_fr 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Vco_m3_at_Tfr 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mn>
            1 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            6 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.39)</p>
     <p>With Qf_fr calculated in §4.6 and Vco_m3_at_Tfr in §4.7.</p>
     <p>So the average neutron flux is equal to (cf. <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 104):</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Thermal_fission_neutron_flux 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Fission_rate 
          </mtext> 
         </mrow> 
         <mrow> 
          <mi>
            ε 
          </mi> 
          <mo>
            × 
          </mo> 
          <mtext>
            Sigma_f_th 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.40)</p>
     <p>The fission rate is divided by ε (calculated in §4.9) to subtract fast fissions. Sigma_f_th is the thermal fission macroscopic cross-section ( 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mo>
          = 
        </mo> 
        <mstyle displaystyle="true"> 
         <munder> 
          <mo>
            ∑ 
          </mo> 
          <mi>
            i 
          </mi> 
         </munder> 
         <mrow> 
          <mi>
            N 
          </mi> 
          <mi>
            i 
          </mi> 
          <mo>
            × 
          </mo> 
          <mi>
            σ 
          </mi> 
          <mi>
            f 
          </mi> 
          <mi>
            i 
          </mi> 
         </mrow> 
        </mstyle> 
       </mrow> 
      </math>, cf. <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 69), detailed in the “D_D_PWR_hybrid_reactor” program.</p>
     <p><u>Final neutrons flux</u></p>
     <p>It will be considered that for K_eff ≤ 0.01, i.e., a fission reactor state with almost no reactivity, the final neutrons flux will be calculated on the basis of the Thermal_fusion_neutron_flux. Reversely for K_eff &gt; 0.01, it will be calculated on the basis of the Thermal_fission_neutron_flux.</p>
     <p>This only applies to the Thorium fuel. For the Uranium (natural or depleted), K_eff is always widely superior to 0.01, so the sole Thermal_fission_neutron_flux is used.</p>
     <p><u>Maximum neutrons flux</u></p>
     <p>Note that about the thorium fuel incineration, in <xref ref-type="bibr" rid="scirp.137109-8">
       [8]
      </xref> (p. 13), it is calculated a maximum neutrons flux equal to 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mn>
          2.0 
        </mn> 
        <mtext>
          E 
        </mtext> 
        <mn>
          14 
        </mn> 
        <mo>
          × 
        </mo> 
        <msqrt> 
         <mrow> 
          <mtext>
            Treactor 
          </mtext> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mtext>
             K 
           </mtext> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            / 
          </mo> 
          <mn>
            300 
          </mn> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </math>, this to avoid an important bypass of the U233 fission. This limit is high and will not be considered in the present reactor design.</p>
    </sec>
    <sec id="s4_11">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.11. Refueling and Fuel Burn-Up</title>
     <p>The fuel reprocessing and refueling are supposed to be done as detailed in <xref ref-type="bibr" rid="scirp.137109-27">
       [27]
      </xref>. So the fission products and the minor actinides (americium, curium, neptunium), are removed from the spent fuel and finally stored.</p>
     <p><u>Note:</u> the Protactinium (Pa) isotopes rapidly disappear, due to their weak radioactive half-life (27 days for the Pa233 and 6.7 hours for the Pa234). So, the quantity of Protactinium isotopes is considered as nil after refueling.</p>
     <p>Not removing the minor actinides Am and Cm would reduce the net electrical power. For example, after 255 years of operation, the loss would be equal to 100% for the natural Uranium and less than 0.1% for the natural Thorium. So, such a hypothesis is not considered, even if the magnitude of this problem for Thorium is weaker.</p>
     <p><u>Note</u>: as Am241 and Cm244 are considered as final actinides (see §4.12), they accumulate. In reality, transmutations continue. The result for natural Uranium (100% loss) is probably exaggerated, but not so much. Even for Thorium, the very slow accumulation of Am241, Cm244 and successors will finish to reduce the reactivity and the net electrical power. However, thanks to this weak accumulation, the refueling of the whole Thorium fuel could be made when the fuel burn-up reaches 100 GWd/t instead of 10 GWd/t.</p>
     <p>Reversely, not removing the Neptunium does not change almost anything in the results, except 0.1% on the final net electrical power with Thorium. So, the Np237 can remain in the fuel, but the other isotopes of the Neptunium rapidly disappear by radioactive decay. However, to simplify, all Neptunium isotopes will be set to 0 after each refueling.</p>
     <p>The Uranium and the Plutonium are extracted (PUREX process, described in <xref ref-type="bibr" rid="scirp.137109-27">
       [27]
      </xref>). For the Thorium, a similar process to extract Thorium called “THOREX” is expected. See from §5.1 to §5.4 for recommendations about these processes.</p>
     <p>To simplify the calculation, it is supposed to be a regular refueling of the whole fuel (and not by 1/3 or 1/4) each time the fuel burn-up (calculated from the previous refueling) passes 10000 MWd/t, so once each 7 to 9 years. Note that this value of 10,000 MWd/t is inferior to the current burn-up limit for PWR fuel assemblies, see <xref ref-type="bibr" rid="scirp.137109-28">
       [28]
      </xref> (pp. 57-58). Moreover, it is supposed that the fuel reprocessing is done immediately and not after years.</p>
     <p>So, after each immediate fuel reprocessing/refueling:</p>
     <p><u>Note</u>: for Thorium, the refueling could possibly be done after a burn-up larger than 10000 MWd/t, because the accumulation of minor actinides is slow and weak.</p>
     <p>The fuel burn-up (Burn_up_MWd_t) is calculated in the following way.</p>
     <p>At each step (one hour of working), the thermal energy produced during this step is calculated, i.e., 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mi>
          Δ 
        </mi> 
        <mtext>
          ThermalEnergy 
        </mtext> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            MJ 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mtext>
          Pth_fission_MW 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mn>
          3600 
        </mn> 
       </mrow> 
      </math>, with Pth_fission_MW calculated in §4.6.</p>
     <p>This energy is added to Energy_generated_MJ_from_the_last_refueling.</p>
     <p>The fuel burn-up in MWd/t is calculated this way:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Burn_up_MWd_t 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Energy_generated_MJ_from_the_last_refueling 
          </mtext> 
         </mrow> 
         <mrow> 
          <mn>
            86400 
          </mn> 
          <mo>
            × 
          </mo> 
          <mtext>
            Fuel_mass_t 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (4.41)</p>
     <p>The fuel mass is calculated from the fuel volume:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Fuel_volume_m3_20_C 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Vco_m3_at_20_C 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mn>
          0.281695 
        </mn> 
       </mrow> 
      </math> (4.42)</p>
     <p>And 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Fuel_mass_t 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mtext>
          Fuel_volume_at_20_C 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          Mean_fuel_specific_gravity 
        </mtext> 
       </mrow> 
      </math> (4.43)</p>
     <p>With Vco_at_20_C calculated in §4.7 and the Mean_fuel_specific_gravity detailed in the “D_D_PWR_hybrid_reactor” program.</p>
     <p>It is also calculated and displayed at each reloading the mass of fuel consumed from the beginning of operation, which reported to the total thermal energy produced, gives the average burn-up of the consumed fuel in MWd/t. A calculation of this average burn-up gives after 255 years of operation, the reactor being considered stabilized:</p>
    </sec>
    <sec id="s4_12">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.12. Fuel Evolution</title>
     <p>In <xref ref-type="fig" rid="fig6">
       Figure 6
      </xref> below, the simplified chain of the managed fuel will be found.</p>
     <p>The calculation of the fuel evolution is repetitive, and so it is not described here. It is detailed in the source code of the “D_D_PWR_hybrid_reactor” program.</p>
     <fig id="fig6" position="float">
      <label>Figure 6</label>
      <caption>
       <title>Figure 6. Simplified evolution chain of a Thorium (Th232) + Uranium (U238+U235) fuel.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId196.jpeg?20241111100729" />
     </fig>
     <p>Note that Am241 and Cm244 are the final minor actinides of this simplified evolution chain. In fact, there are other transmutations of both materials in other minor actinides, but without importance relatively to the target of this document.</p>
     <p>To abstract, the equations are based on two main reactions (see also <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref>, p. 260, for more details):</p>
     <p><u>Note 1</u>: for fissile materials, a neutron absorption can generate either a capture or a fission. The n ◊ 2n reaction also exists at high energies, but it is not considered here.</p>
     <p><u>Note 2</u>: thermal cross-sections σ are supposed to follow a correction in 1/Speed (i.e. σ decreases when the temperature increases), even if it is only approximate compared to reality, so: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Correction_of_ 
        </mtext> 
        <mi>
          σ 
        </mi> 
        <mo>
          = 
        </mo> 
        <msqrt> 
         <mrow> 
          <mfrac> 
           <mrow> 
            <mn>
              293.15 
            </mn> 
           </mrow> 
           <mrow> 
            <mtext>
              Tfr_C 
            </mtext> 
            <mo>
              + 
            </mo> 
            <mn>
              273.15 
            </mn> 
           </mrow> 
          </mfrac> 
         </mrow> 
        </msqrt> 
       </mrow> 
      </math></p>
     <p><u>Note 3</u>: resonance integrals Ia (absorption), If (fission), and Ia-If (capture) are supposed to increase linearly with the temperature (as p the resonance escape probability decreases with the temperature), so</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Correction_of_Ia_If 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Tfr_C 
          </mtext> 
          <mo>
            + 
          </mo> 
          <mn>
            273.15 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            293.15 
          </mn> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math></p>
     <p>The fuel absorption data in the epithermal domain through the resonance integrals are given by <xref ref-type="bibr" rid="scirp.137109-21">
       [21]
      </xref> (pp. 466-467). However, the self-shielding factor which reduces each resonance integral is not known, because it depends on the neutron spectrum. A self-shielding factor of 14 by default is taken, but it is very imprecise.</p>
     <p>For Uranium, these factors have been calibrated to be close to the fuel evolution results given in <xref ref-type="bibr" rid="scirp.137109-29">
       [29]
      </xref> (p. 25), for a PWR. So the calculated Uranium fuel evolution must be considered as not very far away from reality.</p>
     <p><u>Note about comparison between PWR and Candu reactors, with natural Uranium as fuel</u><u>.</u></p>
     <p>Fuel evolution of Candu, as the one given by <xref ref-type="bibr" rid="scirp.137109-26">
       [26]
      </xref> (p. 135), cannot be used for a PWR because its neutron spectrum is mainly only thermal due to the very good moderation, whereas the PWR spectrum is also epithermal for a small part. With the same neutron flux, the production of Plutonium by the PWR is stronger due to this difference in neutron spectrum.</p>
     <p>The initial K_infinite of a Candu reactor is higher than the initial K_infinite of a PWR (about 1.08 versus 0.88), because it is better moderated with heavy water in a large reactor.</p>
     <p>But due to this PWR better production of Plutonium, the K_infinite evolution is different, as the initial increase of K infinite is stronger on a PWR compared to a Candu: 1.08 to 1.09 for a Candu (<xref ref-type="bibr" rid="scirp.137109-26">
       [26]
      </xref>, p. 128) but 0.88 to 1.09 for a PWR according to the author’s calculations.</p>
     <p>Note that the high thermal neutrons flux of Candu reactors (about 1E14 n/(cm<sup>2</sup>∙s)) compared to a PWR (about 3E13 n/(cm<sup>2</sup>.s)) accelerates the process, but does not change much the fuel evolution.</p>
     <p>Of course, there is no example of PWR working with Thorium. However, it has been verified that the Thorium fuel evolution results are coherent with <xref ref-type="fig" rid="fig4">
       Figure 4
      </xref> of <xref ref-type="bibr" rid="scirp.137109-8">
       [8]
      </xref>, which also shows a calculated Thorium fuel evolution. The fuel evolution results given for Thorium must be considered as inaccurate.</p>
    </sec>
    <sec id="s4_13">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>4.13. Description of the Way to Calculate the Hybrid Reactor</title>
     <p>Here is described the global way to calculate the hybrid reactor, as written in the source code of the “D_D_PWR_hybrid_reactor” program.</p>
     <p>For a given fusion pipe radius and a given maximum Beta, the best fusion reactor is calculated according to <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> and to the modifications described from §3.1 to §3.4. Note that the ranges of density of D+ ions and energy injection of particles (D+ ions + electrons) are defined by the user.</p>
     <p>The main results about this fusion reactor, useful for the fission reactor, are described in §3.5 (Qns_2L, Pm_input_W, Pth_fusion_W, P_neutron_2L_W and Pro_n_2_45_MeV).</p>
     <p>Preliminary calculations are done. They are described in §4.2 (Ptr_Be), §4.3 (Pfr_bar_abs and Tfr_C), §4.4 (Yg), §4.5 (K_eff maximum = 0.9, N_fuel and MR). The geometry of the fission reactor is calculated in §4.7 (mainly THco_cm_at_Tfr) using the maximum fission power (Pth_fission_MW) determined in §4.6. The initial K_infinite factor and the non-leakage probability (Pnl) are calculated in §4.9. The minimal thermal neutron flux is calculated in §4.10.</p>
     <p>Once the preliminary calculations are done, it is determined the evolution of the fuel and all the parameters over 100 years by default (255 years maximum), by step of one hour. For one step, it is calculated:</p>
     <p>Each year, it is also given the following pieces of information:</p>
     <p>At the end of the calculation (so after 100 years of working time by default), the final fuel composition (atomic concentrations) is displayed.</p>
     <p>Of course, as the source code is available, the user can modify the information displayed.</p>
    </sec>
   </sec>
   <sec id="s5">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>5. Results and Discussion</title>
    <p>In this chapter, it will be compared the main results obtained with natural Uranium, depleted Uranium, natural Thorium and a 50/50 mixture of natural Uranium and natural Thorium. These main results are:</p>
    <p>Afterward, points to deepen, ways to improve this hybrid reactor and safety aspects will be discussed.</p>
    <sec id="s5_1">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.1. Working with Natural Uranium over 100 Years</title>
     <p>In <xref ref-type="fig" rid="fig7">
       Figure 7
      </xref>, it is displayed the results obtained with natural Uranium as fuel, from 0 to 100 years.</p>
     <p>The discontinuities on K_eff are due to the refueling operations. The initial rise of both parameters is due to the transmutation of U238 in Pu239 before stabilization.</p>
     <p>After stabilization, the net electrical power reaches a value of around 1432 MWe. The net electrical power is constant because the K_eff is limited to 0.9.</p>
     <p>Note that even without borated water, the reactor would remain sub-critical (K_eff &lt; 1) except in year 10, for which it reaches 1.002.</p>
     <p><u>About the fissile Plutonium proliferation</u></p>
     <p>The final composition shows:</p>
     <p>Pu238 = 0.002%, Pu239 = 0.674%, Pu240 = 0.199%, Pu241 = 0.265%, Pu242 = 0.581% and Pu243 = 0.000%</p>
     <p>The fissile materials (Pu239 and Pu241) are present at 0.94%, whereas</p>
     <fig id="fig7" position="float">
      <label>Figure 7</label>
      <caption>
       <title>Figure 7. Main results for natural Uranium with respect to time in years.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId209.jpeg?20241111100730" />
     </fig>
     <p>non-fissile materials are present at 0.78%. The percentage of fissile materials is too much important compared to the non-fissile materials, which might be avoided for obvious reasons.</p>
     <p>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>For this type of reactor and as no Uranium enrichment is required, the PUREX process might be modified so that no separation between Uranium and Plutonium be made. In that case, the Plutonium would be mixed with 98.058% of U238 (non-fissile) and no direct risk with this fuel would exist.</p>
    </sec>
    <sec id="s5_2">
     <title>5.2. Working with Depleted Uranium over 100 Years</title>
     <p>In <xref ref-type="fig" rid="fig8">
       Figure 8
      </xref>, it is displayed the results obtained with depleted Uranium as fuel (0.3% of U235), from 0 to 100 years.</p>
     <fig id="fig8" position="float">
      <label>Figure 8</label>
      <caption>
       <title>Figure 8. Main results for depleted Uranium with respect to time in years.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId210.jpeg?20241111100731" />
     </fig>
     <p>The initial rise of both parameters is stronger than for natural Uranium due a smaller initial U235 concentration (0.30% instead of 0.72%). The initial reactivity is equal to 0.505 versus 0.820 for the natural Uranium. The initial net electrical power is negative for about two years, but afterward, it reaches a stabilized value of around 1431 MWe.</p>
     <p><u>About the fissile Plutonium proliferation</u>: the results are about the same as with natural Uranium (§5.1), so the recommendation not to separate Uranium from Plutonium is the same.</p>
    </sec>
    <sec id="s5_3">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.3. Working with Natural Thorium over 100 Years</title>
     <p>In <xref ref-type="fig" rid="fig9">
       Figure 9
      </xref>, it is displayed the results obtained with natural Thorium as fuel, from 0 to 100 years.</p>
     <p>The initial rise of both parameters is deeper and longer than for depleted Uranium due to an initial zero reactivity and transmutation of the fertile material Th232 in the fissile material U233. The initial net electrical power is negative for the first 18 years, but afterward, it reaches a stabilized, more elevated value than Uranium (1631 MWe instead of 1432 MWe). The net electrical power is constant because the K_eff is limited to 0.9. Note that without borated water, the reactor would remain sub-critical (K_eff &lt; 1) for the first 47 years before being stable around 1.008.</p>
     <fig id="fig9" position="float">
      <label>Figure 9</label>
      <caption>
       <title>
        <xref ref-type="bibr" rid="scirp.137109-"></xref>Figure 9. Main results for natural Thorium with respect to time in years.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId211.jpeg?20241111100731" />
     </fig>
     <p><u>About the fissile Plutonium and Uranium proliferation</u></p>
     <p>The final composition shows for Plutonium:</p>
     <p>Pu238 = 0.007%, Pu239 = 0.003%, Pu240 = 0.001%, Pu241 = 0.001%, Pu242 = 0.002% and Pu243 = 0.000%</p>
     <p>The problem is the same as with natural Uranium but with a much lesser magnitude. However, the recommendation not to separate Uranium from Plutonium remains.</p>
     <p>The final composition shows for Uranium:</p>
     <p>U233 = 1.460%, U234 = 0.857%, U235 = 0.210%, U236 = 0.158%, U237 = 0.000%, U238 = 0.000% and U239 = 0.000%.</p>
     <p>The fissile materials (U233 and U235) are present at 1.670%, whereas non-fissile materials are present at 1.015%. The percentage of fissile materials is too much important compared to the non-fissile materials, which might be avoided for obvious reasons.</p>
     <p>For this type of reactor, the THOREX process might be modified so that no separation between Uranium, Plutonium and Thorium be made. In that case, the fissile Uranium and Plutonium would be mixed with 96.560% of Th232 (non-fissile) and no direct risk with this fuel would exist.</p>
    </sec>
    <sec id="s5_4">
     <title>5.4. Working with a 50/50 Mixture of Natural Uranium and Natural Thorium over 100 Years</title>
     <p>In <xref ref-type="fig" rid="fig10">
       Figure 10
      </xref>, it is displayed the results obtained with a mixture of 50% of natural Uranium (0.36% of U235 and 49.64% of U238) and 50% of natural Thorium, from 0 to 100 years.</p>
     <p>The initial rise of both parameters is due to the transmutation of U238 in Pu239 and Th232 in U233, before stabilization. The initial net electrical power is negative for the first 6 years, but afterward, it reaches a stabilized, more elevated value than Uranium (1532 MWe instead 1432 MWe). Note that without borated water, the</p>
     <fig id="fig10" position="float">
      <label>Figure 10</label>
      <caption>
       <title>Figure 10. Main results for a 50/50 mixture of natural Uranium and natural Thorium with respect to time in years.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId212.jpeg?20241111100731" />
     </fig>
     <p>reactor would remain sub-critical (K_eff &lt; 0.96).</p>
     <p><u>About the fissile Plutonium proliferation</u></p>
     <p>The final composition shows for Plutonium and Uranium:</p>
     <p>Pu238 = 0.005%, Pu239 = 0.335%, Pu240 = 0.099%, Pu241 = 0.133%, Pu242 = 0.292% and Pu243 = 0.000%.</p>
     <p>U233 = 0.738%, U234 = 0.431%, U235 = 0.110%, U236 = 0.092%, U237 = 0.000%, U238 = 48.223% and U239 = 0.000%.</p>
     <p>The problem is the same as with natural Uranium but with a half magnitude. The recommendation not to separate Uranium, Thorium and Plutonium remains, even if in that case the Thorium could be possibly separated thanks to the U238 presence.</p>
    </sec>
    <sec id="s5_5">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.5. Estimation of the Reactor Service Life Limitations Due to the Neutrons Flux</title>
     <p>Due to the neutrons flux, the mechanical characteristics of the Beryllium first wall and the 316LN exterior wall will be progressively altered. The service life of this reactor mainly depends on the service lives of both walls.</p>
     <p><u>Note</u>: the reactor service life also depends, equipment by equipment, on the number of operating transients. This reactor is supposed to work in a steady-state operation to minimize the number of transients.</p>
     <p>As shown below, both service lives are much larger than the minimum expected service life for this reactor, which is supposed equal to 100 years. So, the reactor size could be reduced, if possible, for this aspect of things.</p>
     <p><u>About the Beryllium first wall</u></p>
     <p>The main problem is the generation of 14.06 MeV neutrons due to fusions: see the interaction between neutrons and Beryllium in §4.2. From the default configuration results, about 26% of the neutrons are 14.06 MeV ones, for an average neutrons flux (“SNP”) of 10600 W/m<sup>2</sup>. Let’s suppose that:</p>
     <p>In these conditions, the service life of the first wall will be limited to: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mfrac> 
         <mrow> 
          <mn>
            2 
          </mn> 
          <mtext>
            E 
          </mtext> 
          <mn>
            6 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            10600 
          </mn> 
          <mo>
            × 
          </mo> 
          <mn>
            0.26 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mn>
          726 
        </mn> 
        <mtext>
            
        </mtext> 
        <mtext>
          years 
        </mtext> 
       </mrow> 
      </math></p>
     <p><u>About the 316LN exterior wall</u></p>
     <p>The P4/P’4 PWR was initially designed for service life, mainly depending on the reactor vessel body, of 40 years. The thermal power is equal to 3800 MW and the surface of the vessel in front of the core is equal to about 59 m<sup>2</sup>, whereas they are respectively equal to 6160 MW and 6015 m2 for this reactor in its default configuration.</p>
     <p>The service life for the exterior wall, which is, as first hypothesis, inversely proportional to the thermal power and proportional to the surface receiving the neutrons flux, will be limited to: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mn>
          40 
        </mn> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            3800 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            6160 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            6015 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            59 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          = 
        </mo> 
        <mn>
          2516 
        </mn> 
        <mtext>
            
        </mtext> 
        <mtext>
          years 
        </mtext> 
       </mrow> 
      </math>.</p>
    </sec>
    <sec id="s5_6">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.6. Points to Deepen</title>
     <p>This is a non-exhaustive list of points to deepen. The points to deepen given in <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> could also be consulted, even if they are less critical due to the more realistic fusion configuration used in this document.</p>
    </sec>
    <sec id="s5_7">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.7. Possible Slight Improvement of the Hybrid Reactor by Injection of Tritium with the Deuterium</title>
     <p>This possibility is proposed for information because the gain is weak and the breeding system is complex.</p>
     <p><u>Introduction</u></p>
     <p>Even if it is not indispensable, several percent of Tritium in the Deuterium would boost the fusion reactor.</p>
     <p>In <xref ref-type="fig" rid="fig5">
       Figure 5
      </xref>, it appears that, at 29 keV, the D-T reaction rate is about 80 times the D-D one (and so about 160 times the D-D fusion rate) and even much more for D-He3. The production of Tritium by the PWR associated with the fusion reactor would be very weak, i.e., several g per year, mainly due to “ternary fissions” in the Uranium fuel.</p>
     <p>Now, a part of the Tritium injected (if any) and produced by D-D reaction is lost on the wall. This tritium mixed with other gas, is recovered thanks to the vacuum pumping system. Afterward, the Tritium could be separated from the recovered gas and stored.</p>
     <p>Another more efficient solution would be to install a Tritium breeding blanket (see <xref ref-type="bibr" rid="scirp.137109-30">
       [30]
      </xref> for information), with its Tritium extraction system, at the exterior of the fission reactor between the reflector and the 316LN exterior wall. Of course, this Lithium blanket will be separated from the water due to an exothermic reaction between both.</p>
     <p>The fission neutrons crossing the reflector are slowed down by this one. In the Lithium blanket, these thermal neutrons will generate Tritium, according to the fission reaction between a thermal neutron and the Lithium 6 (<xref ref-type="bibr" rid="scirp.137109-31">
       [31]
      </xref>): n + <sup>6</sup>Li ◊ <sup>4</sup>He + T + 4.78 MeV (kinetic energy).</p>
     <p>The Tritium will be separated from Helium and stored.</p>
     <p>Note that there is no possibility to multiply neutrons inside the Lithium blanket through n ◊ 2n reactions with Beryllium or Lead, because the neutrons are thermal.</p>
     <p>The generated Tritium will be added to the Deuterium gas before being injected as D+ and T+ ions, into the fusion reactor. So, the rate of D-T fusion neutrons will be increased. This gain will permit an increase in the net electrical power.</p>
     <p>See the sectional view in <xref ref-type="fig" rid="fig11">
       Figure 11
      </xref> and compare it with the sectional view in <xref ref-type="fig" rid="fig2">
       Figure 2
      </xref>.</p>
     <p>The TBR (Tritium Breeding Ratio) of this Lithium blanket is close but inferior to 1, i.e., a neutron entering the Lithium blanket will generate, on average, a bit less than one atom of Tritium.</p>
     <fig id="fig11" position="float">
      <label>Figure 11</label>
      <caption>
       <title>Figure 11. Sectional view at the level of the straight parts.</title>
      </caption>
      <graphic mimetype="image" position="float" xlink:type="simple" xlink:href="https://html.scirp.org/file/1090543-rId217.jpeg?20241111100733" />
     </fig>
     <p><u>Estimation of the gain due to this Tritium contribution</u></p>
     <p>The rate of atoms of Tritium (per s and per m<sup>3</sup> of fusion reactor), generated by the Lithium blanket can be written: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          QTgen_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mtext>
          Qfnm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          Kn 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          TBR 
        </mtext> 
       </mrow> 
      </math> (equation 5.1)</p>
     <p>With Qfnm3 the rate of fusion neutrons (at 2.45 and 14.06 MeV) generated per s and per m<sup>3</sup> of fusion reactor (§3.5): 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Qfnm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mtext>
          QfDDm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          / 
        </mo> 
        <mn>
          2 
        </mn> 
        <mo>
          + 
        </mo> 
        <mtext>
          QfDTm 
        </mtext> 
        <mn>
          3 
        </mn> 
       </mrow> 
      </math> (equation 3.9)</p>
     <p>From §4.2, §4.6 and §4.9, it can be calculated the Kn factor giving the number of fission neutrons reaching the Lithium blanket for one fusion neutron:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Kn 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mn>
            10 
          </mn> 
         </mrow> 
         <mrow> 
          <mn>
            11 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            Ptr_Be 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            1-K_eff 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Mean_Nu 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mtext>
            Pnl 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
       </mrow> 
      </math> (5.1)</p>
     <p>Ptr_Be (§4.2) varies between 0.915 with 100% of 2.45 MeV neutrons and 1.313 with 100% of 14.06 MeV neutrons. (1-Pnl) represents the probability of a fission neutron to leak the fission reactor with 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          Pnl 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            K_infinite 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (from §4.9). 10/11 is the ratio between the fusion volume of the straight parts and the total fusion volume.</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            1 
          </mn> 
          <mo>
            − 
          </mo> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            K_eff 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            Mean_Nu 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> is the neutrons multiplication factor due to the sub-critical fission reactor. It is reminded that the maximum K_eff has been supposed equal to 0.9 in §4.5.</p>
     <p>Now according to the §2.2.6 of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref> and without considering the charge exchanges (§3.4), it can be written, at equilibrium, when the loss of Tritium is equal to the gain of Tritium:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          QiTm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          + 
        </mo> 
        <mtext>
          QTgen_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            nT 
          </mtext> 
         </mrow> 
         <mrow> 
          <mtext>
            TDexp 
          </mtext> 
         </mrow> 
        </mfrac> 
        <mo>
          + 
        </mo> 
        <mrow> 
         <mo>
           ( 
         </mo> 
         <mrow> 
          <mtext>
            nT 
          </mtext> 
          <mo>
            × 
          </mo> 
          <mi>
            γ 
          </mi> 
          <mtext>
            fDT 
          </mtext> 
         </mrow> 
         <mo>
           ) 
         </mo> 
        </mrow> 
        <mo>
          = 
        </mo> 
        <mtext>
          nT 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mrow> 
         <mo>
           [ 
         </mo> 
         <mrow> 
          <mfrac> 
           <mn>
             1 
           </mn> 
           <mrow> 
            <mtext>
              TDexp 
            </mtext> 
           </mrow> 
          </mfrac> 
          <mo>
            + 
          </mo> 
          <mi>
            γ 
          </mi> 
          <mtext>
            fDT 
          </mtext> 
         </mrow> 
         <mo>
           ] 
         </mo> 
        </mrow> 
       </mrow> 
      </math></p>
     <p>so it can be deduced the density of tritium atoms nT:</p>
     <p>
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          nT 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mrow> 
          <mtext>
            QiTm 
          </mtext> 
          <mn>
            3 
          </mn> 
          <mo>
            + 
          </mo> 
          <mtext>
            QTgen_m 
          </mtext> 
          <mn>
            3 
          </mn> 
         </mrow> 
         <mrow> 
          <mrow> 
           <mo>
             ( 
           </mo> 
           <mrow> 
            <mn>
              1 
            </mn> 
            <mo>
              / 
            </mo> 
            <mtext>
              TD 
            </mtext> 
            <mi>
              exp 
            </mi> 
           </mrow> 
           <mo>
             ) 
           </mo> 
          </mrow> 
          <mo>
            + 
          </mo> 
          <mi>
            γ 
          </mi> 
          <mtext>
            fDT 
          </mtext> 
         </mrow> 
        </mfrac> 
       </mrow> 
      </math> (5.2),</p>
     <p>from which it will be calculated the rate of D-T fusions (QfDTm3, §2.2.6 of <xref ref-type="bibr" rid="scirp.137109-1">
       [1]
      </xref>), which is proportional to nT. The larger is QTgen_m3 and hence Kn, the larger is nT and the rate of D-T fusions QfDTm3. Note that Qfnm3 depends on QfDTm3, so the process is iterative and converges towards a given value.</p>
     <p>The problem is that the fusion reactor is calculated before the fission reactor, so Kn is not known.</p>
     <p>To avoid a too complex calculation, it will be supposed a Kn_supposed factor. Then, the calculation will be done by the program. The real average Kn_average will be given once the fission reactor calculated.</p>
     <p>Kn_supposed must be close to Kn_average.</p>
     <p>A basic value for Kn is 0.16 with Ptr_Be = 1, K_eff = 0.9, Mean_Nu = 2.5, Pnl = 0.95, which is not much. To have a larger Kn, if K_infinite is sufficiently large, the possibilities are:</p>
     <p>Moreover, a more accurate calculation of the neutrons multiplication in the Beryllium wall than the one conservative, done in §4.2 will be welcome.</p>
     <p><u>Example</u></p>
     <p>First, let’s suppose that, including the Tritium recovered by vacuum pumping, the global TBR reaches 1.</p>
     <p>Now, let’s suppose a radius Rp = 100 cm. With the K_eff limited to 0.9, the average net electrical power is equal to 46 MW, for a mechanical gain Q equal to 0.062.</p>
     <p>With the generation of Tritium in service (i.e., TEST_WITH_ADDED_TRITIUM_TO_THE_DEUTERIUM = TRUE in the program):</p>
     <p>The gain on net power is equal to 16 MW, which is weak for such complex equipment.</p>
     <p><u>Lithium blanket inside </u><u>both</u><u> half-toruses</u></p>
     <p>To increase the Tritium production, a Lithium blanket could also be installed inside both half-toruses to generate Tritium. The rate of atoms of Tritium, generated by this Lithium blanket would be: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          QT'gen_m 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          = 
        </mo> 
        <mtext>
          Qfnm 
        </mtext> 
        <mn>
          3 
        </mn> 
        <mo>
          × 
        </mo> 
        <mtext>
          K'n 
        </mtext> 
        <mo>
          × 
        </mo> 
        <mtext>
          TBR 
        </mtext> 
       </mrow> 
      </math>, with the K'n factor giving the number of fission neutrons reaching the Lithium blanket for one fusion neutron, for both half-toruses: 
      <math display="inline" xmlns="http://www.w3.org/1998/Math/MathML"> <mrow> 
        <mtext>
          K'n 
        </mtext> 
        <mo>
          = 
        </mo> 
        <mfrac> 
         <mn>
           1 
         </mn> 
         <mrow> 
          <mn>
            11 
          </mn> 
         </mrow> 
        </mfrac> 
        <mo>
          × 
        </mo> 
        <mtext>
          Ptr_Be 
        </mtext> 
       </mrow> 
      </math>.</p>
     <p>In that case, the space just above the interior beryllium wall will be filled with light water (cooled by an exterior system) to slow down and thermalize the neutrons up to the Lithium blanket.</p>
    </sec>
    <sec id="s5_8">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.8. Other Improvements of the Hybrid Reactor</title>
     <p>Below is a non-exhaustive list of possible improvements to this hybrid reactor.</p>
    </sec>
    <sec id="s5_9">
     <title>
      <xref ref-type="bibr" rid="scirp.137109-"></xref>5.9. Safety</title>
     <p><u>Main nuclear accident to mitigate</u></p>
     <p>This preliminary accident analysis is to be considered very rough, as it is a very complex subject.</p>
     <p>The K_eff multiplication factor being limited to a maximum of 0.9, and as there are no emergency shutdown rods, no criticality accident and no failure of the emergency trip have to be considered. So the probability of occurrence of accidents supposing partial or total failures of the emergency trip and leading to core meltdown, such as Anticipated Transient Without Scram (ATWS), Loss Of Coolant Accident (LOCA) and Steam Line Break (SLB), must be considered as much lower.</p>
     <p>Note that if the fission reactor must be stopped, it will be stopped by a fusion reactor drop, which is the source of neutrons. Practically, it will be done by either stopping the particles injection and, possibly, by injecting neutral gas to extinguish fusions. In this case, the fission reactor will be naturally stopped in several seconds.</p>
     <p>An analysis based on a Probabilistic Risk Assessment of the most probable (or, better say the least improbable) accidents for a PWR is given in <xref ref-type="bibr" rid="scirp.137109-34">
       [34]
      </xref> (p. 19). It appears that without APRP (LOCA), ATWS and RTV (SLB), the most probable accident (at 75%) would be the H3 accident (Total loss of external and internal electrical power). To date, several systems exist to mitigate this accident (turbine-driven auxiliary pumps, passive cooling system, exterior diesel generator sets, exterior cold sources, etc). Consequently, the core meltdown probability is extremely low.</p>
     <p><u>Fissile Uranium and Plutonium proliferation</u></p>
     <p>As explained from §5.1 to §5.4, for this type of reactor, the fuel reprocessing might be such that no separation between Uranium, Plutonium and Thorium be made. In that case, no direct risk with the fuel would exist.</p>
     <p>Moreover, no enrichment is needed for this type of reactor, which also limits proliferation.</p>
    </sec>
   </sec>
   <sec id="s6">
    <title>
     <xref ref-type="bibr" rid="scirp.137109-"></xref>6. Conclusions</title>
    <p>This relatively simple hybrid reactor has been described in §2. Afterward, it has been modeled:</p>
    <p>From §5.1 to §5.4, the main results have been presented about the working of this reactor with different types of fuel, i.e., natural Uranium, depleted Uranium, natural Thorium, or a 50/50 mixture of natural Uranium and natural Thorium. It appears that this reactor is able to successfully incinerate any natural or depleted nuclear fuel for thousands of years of world consumption, as shown in §1.1.</p>
    <p>The net electrical power with the Thorium fuel, at equilibrium, is better than the one with the Uranium fuel, even if at the beginning of the Thorium incineration, this reactor is an electricity consumer (§5.3). It must also be added that Thorium fuel produces much fewer minor actinides (americium and curium) than the Uranium fuel, which would permit to space of the reloading/reprocessing operations (see §4.11) and to reduce the volume and the toxicity of waste.</p>
    <p>The net electrical power roughly depends on the reactor volume. For example, in this paper, the default configuration is a plant producing about 1400 MWe as a big fission plant, the fusion radius being equal to 2 m. According to the same models, the power would be around 440 MWe for a fusion radius of 1.5 m and around 3000 MWe for a fusion radius of 2.5 m, but equal to 46 MWe for a fusion radius of 1 m.</p>
    <p>Now, for a radius of 2 m, the reactor is 200 m long, which is rather large. To reduce the size of such a reactor for the same net electrical power, one could increase the Beta factor (§3.2) if possible or, more slightly, the maximum K_eff (§4.5).</p>
    <p>The expected life (§5.5) is equal or superior to 100 years, due to the low neutrons flux on the first wall in Beryllium and on the exterior wall in 316LN.</p>
    <p>This reactor is safer than a PWR reactor due to its subcriticality (§5.9). Moreover, the absence of U235 enrichment and the uselessness of separating the Uranium, Thorium and Plutonium in the reprocessing operation makes the fuel safer in regard to proliferation. It must also be added that the final waste is constituted by fission products, minor actinides (mainly americium and curium), without any spent fuel (i.e., Uranium, Plutonium or Thorium).</p>
    <p>Points to deepen and improvements of this reactor from §5.5 to §5.8 complete the analysis of this hybrid reactor.</p>
    <p>The presented results are orders of magnitude due to simplified modeling, but they are sufficient to consider the possibility of a functional hybrid reactor.</p>
   </sec>
  </sec>
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