<?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><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjnst.2013.31001</article-id><article-id pub-id-type="publisher-id">WJNST-27465</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  On the Build-Up Factor from the Multi-Group Neutron Diffusion Equation with Cylindrical Symmetry
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ulio</surname><given-names>Cesar Lombaldo Fernandes</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marco</surname><given-names>Túllio Vilhena</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bardo</surname><given-names>Ernst Bodmann</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Volnei</surname><given-names>Borges</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>DepartmentofAppliedMath, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>julio.lombaldo@ufrgs.br(UCLF)</email>;<email>vilhena@ufrgs.br(MTV)</email>;<email>bado.bodmann@ufrgs.br(BEB)</email>;<email>borges@ufrgs.br(VB)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>29</day><month>01</month><year>2013</year></pub-date><volume>03</volume><issue>01</issue><fpage>1</fpage><lpage>5</lpage><history><date date-type="received"><day>August</day>	<month>9,</month>	<year>2012</year></date><date date-type="rev-recd"><day>October</day>	<month>7,</month>	<year>2012</year>	</date><date date-type="accepted"><day>October</day>	<month>21,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; 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><p>
 
 
   We consider the time dependent neutron diffusion equation for one energy group in cylinder coordinates, assuming translational symmetry along the cylinder axis. This problem for a specific energy group is solved analytically applying the Hankel transform in the radial coordinate r. Our special interest rests in the build-up factor for a time dependent linear neutron source aligned with the cylinder axis, which in the limit of zero decay constant reproduces also the static case. The new approach to solve the diffusion equation by integral transform technique is presented and results for several parameter sets and truncation in the solution for the flux and build-up factor are shown and found to be compatible to those of literature [1,2]. 
 
</p></abstract><kwd-group><kwd>Build-Up Factor</kwd><kwd> Cylindrical Geometry; Hankel Transform</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Energy production and environmental issues are strongly related and even though recent events have put nuclear energy on the black list of energy sources, it will recover its role in world’s energy production matrices. In this sense it remains meaningful to search for progress in topics related to nuclear reactor theory, especially by virtue of recent efforts in innovative nuclear reactor technology. As a contribution in this line we develop an analytical method to determine the build-up factor for neutrons, the description of neutron distributions inside the nuclear reactor core. Note, that other applications with this method are possible such as radiation protection, nuclear medicine, among others, see the works [3-5]. The mathematical model that serves as our starting point is motivated by the S<sub>2</sub> approximation of the Boltzmann equation, i.e. the diffusion equation [<xref ref-type="bibr" rid="scirp.27465-ref6">6</xref>]. This equation represents the balance between production and loss of these particles, described in the next section. In Sections 2 and 3 we solve this problem in an analytical fashion using the finite Hankel Transform, which is appropriate for problems represented in cylindrical coordinates, following the idea of the solution of this kind of problem in Cartesian geometry [7,8].</p></sec><sec id="s2"><title>2. Neutron Diffusion</title><p>We consider the time dependent neutron diffusion equation for one energy group in cylinder coordinates, assuming translational symmetry along the cylinder axis</p><disp-formula id="scirp.27465-formula618"><label>(1)</label><graphic position="anchor" xlink:href="1-1090077\a76fc6bd-652c-4b54-8933-bce2536d8eb8.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="1-1090077\0c722ea3-60eb-4b70-8207-bead122a3a66.jpg" /> is the scalar neutron flux, D is the diffusion coefficient for neutrons, <img src="1-1090077\afd40ac1-39da-4698-a1f7-15a4e2b74a4c.jpg" />is the radial part of the elliptic operator, given by</p><disp-formula id="scirp.27465-formula619"><label>(2)</label><graphic position="anchor" xlink:href="1-1090077\10560e9a-e9ef-4dda-acf8-82d605e7debb.jpg"  xlink:type="simple"/></disp-formula><p>The <img src="1-1090077\c94f28f6-2cfc-462f-9733-bff059ba91b3.jpg" /> is the macroscopic removal cross section and <img src="1-1090077\b5156053-5429-4fbb-b59c-7f4599afb4e9.jpg" /> is the source of the problem, that depends on r and t, respectively. Equation (1) is subject to the following boundary conditions</p><disp-formula id="scirp.27465-formula620"><label>(3)</label><graphic position="anchor" xlink:href="1-1090077\0c7238ca-17c5-40e6-8bfc-115d6efb150a.jpg"  xlink:type="simple"/></disp-formula><p>This problem for one energy group may be solved analytically applying the Hankel transform in the radial coordinate r in cylindrical geometry.</p></sec><sec id="s3"><title>3. Solution by Finite Hankel Transform</title><p>Next, we apply the Finite Hankel transform of order zero to (1), making use of some properties of the transform. Recalling, that the Hankel transform of order p has the definition,</p><disp-formula id="scirp.27465-formula621"><label>(4)</label><graphic position="anchor" xlink:href="1-1090077\4bf3ee17-31e8-4f50-9579-a32dcce764db.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-1090077\b2f9b020-0ad4-4f3e-856b-d43089951db2.jpg" /> are values such that <img src="1-1090077\1cacb93c-8151-4c16-a352-4e78e1352e11.jpg" /> for<img src="1-1090077\a54ce0f0-2272-410d-acff-1f46893e6b91.jpg" />, and the inversion is given by</p><disp-formula id="scirp.27465-formula622"><label>(5)</label><graphic position="anchor" xlink:href="1-1090077\89adb712-427d-4181-b73a-ec86a208e986.jpg"  xlink:type="simple"/></disp-formula><p>Differently, than in other applications, where the transform has an infinite upper limit, here the integral has an upper limit R due to the assumption that the flux outside the cylinder with radius R is zero and especially <img src="1-1090077\2d074993-51f0-475b-a06f-1c87b97cffef.jpg" /> holds. Since the neutron flux is related to a distribution means that <img src="1-1090077\70c38a3c-5dcb-4ea4-bb3b-ec32c4192634.jpg" /> is limited. Our special interest is in the build-up factor for the unique initial condition<img src="1-1090077\87048941-b5a4-4f08-9558-8317ec33bd60.jpg" />. Upon multiplying both sides of (1) by<img src="1-1090077\3144528a-47b3-4ce8-8371-8f112a2babe3.jpg" />, and integrating from 0 to the radius R, we obtain</p><disp-formula id="scirp.27465-formula623"><label>(6)</label><graphic position="anchor" xlink:href="1-1090077\39cfec7d-8452-45d5-9c6a-102033e0bc53.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-1090077\27678610-5be6-435a-95ed-8db41313e52a.jpg" /> is the source term of the problem. Using the transformed quantities (6) can be rewritten</p><disp-formula id="scirp.27465-formula624"><label>(7)</label><graphic position="anchor" xlink:href="1-1090077\f4dee2d0-5b77-4076-a9d7-c28c8124e317.jpg"  xlink:type="simple"/></disp-formula><p>The integral containing the spatial derivative may be cast into an expression containing transformed quantities using integration by parts,</p><disp-formula id="scirp.27465-formula625"><label>(8)</label><graphic position="anchor" xlink:href="1-1090077\c96e682c-445c-4e33-81e0-4529f54ed258.jpg"  xlink:type="simple"/></disp-formula><p>which further simplifies due to the choice of <img src="1-1090077\3462106d-23dd-49eb-8659-e00dd3d269e0.jpg" /> such that <img src="1-1090077\10d1ce65-6607-4828-b5a4-0468fd2121d8.jpg" /> and implies that the first term of the right side in (8) vanishes. Therefore,</p><disp-formula id="scirp.27465-formula626"><label>(9)</label><graphic position="anchor" xlink:href="1-1090077\bf8c2f87-f827-49a0-8890-fe2a49830448.jpg"  xlink:type="simple"/></disp-formula><p>which by virtue of</p><disp-formula id="scirp.27465-formula627"><label>(10)</label><graphic position="anchor" xlink:href="1-1090077\4bc9cf77-4cad-4dfb-90de-2d6654c4a490.jpg"  xlink:type="simple"/></disp-formula><p>reduces to</p><disp-formula id="scirp.27465-formula628"><label>(11)</label><graphic position="anchor" xlink:href="1-1090077\f7b103f3-db61-46df-ab4e-9872480dacb2.jpg"  xlink:type="simple"/></disp-formula><p>This equation is subject to the initial condition <img src="1-1090077\5cfa0759-25e5-4dbd-8334-93e19c3474da.jpg" /> because <img src="1-1090077\101e09ea-ab6a-4d9b-b8ae-03d8c76db5b5.jpg" /> and has the solution,</p><disp-formula id="scirp.27465-formula629"><label>(12)</label><graphic position="anchor" xlink:href="1-1090077\f59e7da0-7b65-45bb-aa64-9eaaa76fa5b1.jpg"  xlink:type="simple"/></disp-formula><p>with,</p><disp-formula id="scirp.27465-formula630"><label>(13)</label><graphic position="anchor" xlink:href="1-1090077\4f75cbde-3644-46a6-9396-26098ad2da92.jpg"  xlink:type="simple"/></disp-formula><p>The inversion may be obtained by the use of the definition of the inversion (5) applied to Equation (12). Thus, we obtain the result</p><disp-formula id="scirp.27465-formula631"><label>(14)</label><graphic position="anchor" xlink:href="1-1090077\952456f2-0f67-4324-975a-505f1bced745.jpg"  xlink:type="simple"/></disp-formula><p>and expressed in terms of Equation (12) is</p><disp-formula id="scirp.27465-formula632"><label>(15)</label><graphic position="anchor" xlink:href="1-1090077\ca251f9a-501e-4f77-950d-f32b711a9ff1.jpg"  xlink:type="simple"/></disp-formula><p>that is the solution for the group g. For example, if we consider a fixed source, in this case, we have a source without time dependence, and the inversion (15), can be written as</p><disp-formula id="scirp.27465-formula633"><label>(16)</label><graphic position="anchor" xlink:href="1-1090077\6ac3bbbf-b932-4409-b470-498d38b96f32.jpg"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.27465-formula634"><label>(17)</label><graphic position="anchor" xlink:href="1-1090077\940228a4-0fd0-44b0-ba02-92a2767dd580.jpg"  xlink:type="simple"/></disp-formula><p>and therefore, the final expression for the flux is</p><disp-formula id="scirp.27465-formula635"><label>(18)</label><graphic position="anchor" xlink:href="1-1090077\d0d8eea8-80f0-480c-8ea9-81b25ad3694d.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s4"><title>4. Infinite Line Source Distribution</title><p>We consider now as a source a string that coincides with the centre of the cylinder and may be represented by the Delta Function <img src="1-1090077\a44c93d1-0e86-4ca0-972c-fb7c01ca9d91.jpg" /> (in cylindrical case), which is defined to be zero for all values of r except at r = 0. The integral of <img src="1-1090077\0a9daa13-ab04-4093-a753-d1c6972ca279.jpg" /> is finite, provided r = 0 lies in the range of integration, and the value of the integral is taken to be unity. In order to treat the special case, where r = 0 lies at the border of the interval we recall, that for any compact set <img src="1-1090077\f8e1efbc-2691-4458-992b-a6463ac55f1a.jpg" /> with<img src="1-1090077\09a2ec72-afeb-4895-a6a5-173cafe0d543.jpg" />, that is a compact support for<img src="1-1090077\46a58965-066f-47d2-8db7-16a71a458c93.jpg" />.</p><disp-formula id="scirp.27465-formula636"><label>(19)</label><graphic position="anchor" xlink:href="1-1090077\be8a6dc9-8c4a-4cd8-8351-0baa71559d65.jpg"  xlink:type="simple"/></disp-formula><p>holds as usual, since r = 0 lies truly in the interval. In the case where r = 0 lies at the interval limit, the following limit shall be applied to determine the integral property from above.</p><disp-formula id="scirp.27465-formula637"><label>(20)</label><graphic position="anchor" xlink:href="1-1090077\84c5a68b-f2ee-435b-ba3e-ae90bd4e494d.jpg"  xlink:type="simple"/></disp-formula><p>The Hankel transformed expression for the source as well as in (13). If we have the source has time dependence, as for instance the classical example from reference [<xref ref-type="bibr" rid="scirp.27465-ref9">9</xref>]</p><disp-formula id="scirp.27465-formula638"><label>(21)</label><graphic position="anchor" xlink:href="1-1090077\a51afa8c-3057-4d23-8635-18cded937c18.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-1090077\66197ffe-404b-4676-a7bf-64fde0437435.jpg" /> is the initial value for the source, and <img src="1-1090077\7d9707b3-b322-44e8-9cb5-dd02db86d8dc.jpg" /> is the decay constant, then for<img src="1-1090077\efd24f52-1727-4ff2-ae0c-e882352b5991.jpg" />.</p><disp-formula id="scirp.27465-formula639"><label>(22)</label><graphic position="anchor" xlink:href="1-1090077\ad34c50c-c2d5-4617-a076-2d68e502c44f.jpg"  xlink:type="simple"/></disp-formula><p>Finally, we can express the final solution for the flux, making use of the inversion using (22), yields then</p><disp-formula id="scirp.27465-formula640"><label>(23)</label><graphic position="anchor" xlink:href="1-1090077\487d1ca5-fee9-4f54-bf2b-f32aef527768.jpg"  xlink:type="simple"/></disp-formula><p>The integral in the previous equation may be solved,</p><disp-formula id="scirp.27465-formula641"><label>(24)</label><graphic position="anchor" xlink:href="1-1090077\2c057d0f-88d2-40d6-af60-7a6a9d382302.jpg"  xlink:type="simple"/></disp-formula><p>so that the final solution reads</p><disp-formula id="scirp.27465-formula642"><label>(25)</label><graphic position="anchor" xlink:href="1-1090077\114e7d1e-92ab-4ffc-a4d7-00a1cf7cd069.jpg"  xlink:type="simple"/></disp-formula><p>The time dependent source solution also includes the time independent source term upon taking the limit<img src="1-1090077\1f4dbf31-8fe9-40c6-813c-16bf6a9c2b2e.jpg" />.</p></sec><sec id="s5"><title>5. Analysis of Build-Up Factor</title><p>The build-up factor have been calculated for different response functions that have impact on the design of fuel element distribution. The composition used in this work is that used in the Mirror Advanced Reactor Study (MARS) design. The build-up factor for the response function from an infinite line source is defined as</p><disp-formula id="scirp.27465-formula643"><label>(26)</label><graphic position="anchor" xlink:href="1-1090077\ea3a0fc2-cd88-43ee-82b7-de3fe0fc8129.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-1090077\4460a32c-6a8f-4239-b9eb-c08902fea8cf.jpg" /> is a unit height of the cylinder. The use of the unit length along the cylinder axis is necessary, due to the fact that we considered an infinite cylinder. In our case, we will consider the response function being the flux inside the cylinder divided by the decay constant in order to render the build-up factor dimensionless</p><disp-formula id="scirp.27465-formula644"><label>(27)</label><graphic position="anchor" xlink:href="1-1090077\a3cd3008-4db5-45bf-84ed-0f2e760f397b.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="1-1090077\7c4371a0-bbff-4b81-bd3e-ede9008dc3a7.jpg" /> is the total macroscopic cross section. Therefore, the build-up factor in this case in terms of the ratio of the flux including scattering by the flux without scattering is</p><disp-formula id="scirp.27465-formula645"><label>(28)</label><graphic position="anchor" xlink:href="1-1090077\1f0e0be7-1e1e-434a-b051-04729e205e34.jpg"  xlink:type="simple"/></disp-formula><p>As the material thickness increases from zero to a few mean free paths, the energy spectra of neutrons change considerably. Different build-up factors obtained depend on the energy dependence of cross sections for the different response functions. However, after a few mean free paths, the neutron spectra assume fixed shapes. This stems from the fact that the mean free path for a fission source of neutrons is larger than for lower energy neutrons, as thermal neutrons for instance. This results in the same build-up factor variation with the material thickness regardless of the response function. In <xref ref-type="fig" rid="fig1">Figure 1</xref> we show the correlation of the build-up factor with the radius of our cylinder.</p></sec><sec id="s6"><title>6. Results</title><p>In this section we present a selection of results for several parameter sets and truncation N = 10 in the solution for the flux and build-up factor. The results are comparable to those from other authors.</p><p>The results for the fluxes depending on the parameter choice are shown in Figures 2-5.</p></sec><sec id="s7"><title>7. Conclusion</title><p>In this work, we established the existence for the time dependent neutron flux and build-up factor solution of the time dependent neutron diffusion problem in cylindrical geometry using the Hankel transform for a linear source aligned with the cylinder axis. The obtained solution applies to the time dependent case as well as the time independent case if the decay constant is taken in the zero limit. Since existence and uniqueness of the solution</p><p>is guaranteed by the Cauchy-Kovalewsky theorem, that includes the present equation as a special case, we showed a new approach to solve the diffusion equation by integral transform technique. This procedure allows</p><p>us to generate a function library that efficiently supplies with these solutions, where only the physical and geometrical parameters need to be specified. Furthermore, this method has the advantage, that for numerical purposes the solution may be considered quasi exact, once an adequate number of terms of the solution expansion is taken into account. An error analysis that will specify the truncation index is currently in progress. It is noteworthy, that no numerical errors have to be taken care of due to the analytical character of the solution. Finally motivated by the preliminary good results attained by this methodology, in a forthcoming paper we shall present results for a heterogeneous problem with regions of different physical properties.</p></sec><sec id="s8"><title>8. Acknowledgements</title><p>The authors are gratefully to CNPq (Conselho Nacional de Desenvolvimento Cient&#237;fico e Tecnol&#243;gico) for the partial financial support of this work. 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