<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2017.83025</article-id><article-id pub-id-type="publisher-id">JMP-74465</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Characterizing Atomic Interactions in Interstitial Non-Stoichiometric Compounds by Statistical Thermodynamics: Engineering Usage of Estimated Values of Statistical Thermodynamic Parameters
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nobumitsu</surname><given-names>Shohoji</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>LEN-Laboratório de Energia, LNEG-Laboratório Nacional de Energia e Geologia, Lisboa, Portugal</addr-line></aff><author-notes><corresp id="cor1">* E-mail:</corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>02</month><year>2017</year></pub-date><volume>08</volume><issue>03</issue><fpage>365</fpage><lpage>381</lpage><history><date date-type="received"><day>November</day>	<month>22,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>February</month>	<year>25,</year>	</date><date date-type="accepted"><day>February</day>	<month>28,</month>	<year>2017</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>
 
 
  Statistical thermodynamics allows us to estimate atomistic interactions in interstitial non-stoichiometric compounds 
  <em>MX</em>
  <sub><em>x</em></sub> through analysis of experimentally determined pressure-temperature-composition (
  <em>PTC</em>) relationships for 
  <em>MX</em>
  <sub><em>x</em></sub> being in equilibrium with X
  <sub>2</sub> in gaseous state 
  <em>(X=H,N,P or S)</em> or for non-stoichiometric carbide MCx being in equilibrium with excess C. In case of analysis for 
  <em>MC</em>
  <sub><em>x</em></sub>, chemical activity 
  <em>a(C)</em> of 
  <em>C</em> in place of partial pressure 
  <em>p(X</em>
  <sub><em>2</em></sub>
  <em>)</em> of 
  <em>X</em>
  <sub><em>2</em></sub> gas must be known. On statistical modelling of crystal lattice structure for 
  <em>MX</em>
  <sub><em>x</em></sub>, an a priori assumption of constant nearest-neighbour 
  <em>X-X</em> interaction energy 
  <em>E(X-X</em>
  <em>)</em> within a homogeneity composition range at arbitrary temperature
  <em> T</em> was accepted to determine number 
  <em>θ</em> of available interstitial sites for occupation by 
  <em>X</em> atoms per 
  <em>M</em> atom. Values of interaction parame-ters estimated as such appear rational and realistic noting consistency of the values for 
  <em>M’s</em> in the same group in the Periodic Table of the Elements and compatibility with enthalpy values evaluated by conventional thermodynamic approach. Engineering insights gained for 
  <em>MX</em>
  <sub><em>x</em></sub> through analysis of atomistic interaction parameter values evaluated by the statistical thermodynamics are reviewed comprehensively in this paper. 
  <em>M</em> might be substitutional alloy 
  <em>A</em>
  <sub><em>1-y</em></sub>
  <em>B</em>
  <sub><em>y</em></sub> composed of constituents, 
  <em>A </em>and 
  <em>B,</em> or
  <em> MZ</em>
  <sub><em>z</em></sub> containing another interstitial constituent
  <em> Z</em> besides
  <em> X</em>. Insights acquired from this line of statistical thermodynamic analysis appear to be of pragmatic use for advanced alloy design as shall be demonstrated hereafter.
 
</p></abstract><kwd-group><kwd>Statistical Thermodynamics</kwd><kwd> Non-Stoichiometry</kwd><kwd> Interstitial Compound</kwd><kwd>  Hydride</kwd><kwd> Nitride</kwd><kwd> Carbide</kwd><kwd> Phosphide</kwd><kwd> Sulfide</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Statistical thermodynamic analysis procedures were comprehensively summarized by Fowler and Guggenheim in a classical monograph published in 1949 [<xref ref-type="bibr" rid="scirp.74465-ref1">1</xref>] . Statistical thermodynamics is considered as a bridge connecting between invisible atomistic scale microscopic world and experimentally observable macroscopic state for interstitial non-stoichiometric compound MX<sub>x</sub> possessing composition <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x8.png" xlink:type="simple"/></inline-formula> being in equilibrium with X<sub>2</sub> gas at partial pressure <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x9.png" xlink:type="simple"/></inline-formula> at temperature T. By statistical thermodynamic analysis of equilibrium pressure-temperature-composition (PTC) relationships for MX<sub>x</sub>, nearest-neigh- bour atomic interaction energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x10.png" xlink:type="simple"/></inline-formula> between i and j atoms and atomic partition function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x11.png" xlink:type="simple"/></inline-formula> of constituent i in MX<sub>x</sub> might be calculated<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x12.png" xlink:type="simple"/></inline-formula>.</p><p>Statistical thermodynamic parameters evaluated for extensive range of interstitial non-stoichiometric compounds including hydride, carbide, nitride, phosphide and sulfide were compiled in a monograph published by the author [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] that included calculation results reported by 2012 [<xref ref-type="bibr" rid="scirp.74465-ref3">3</xref>] - [<xref ref-type="bibr" rid="scirp.74465-ref46">46</xref>] . All these analyses [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] - [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] were made accepting an a priori assumption of constant interaction energy <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x13.png" xlink:type="simple"/></inline-formula> between nearest-neighbour interstitial atoms X within a homogeneity composition range of MX<sub>x</sub> lattice at arbitrary T. Parameter values estimated for M’s in the same group in the Periodic <xref ref-type="table" rid="table">Table </xref>of the Elements for given X were comparable to each other. This evidence appeared to support validity of the a priori assumption of the constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x14.png" xlink:type="simple"/></inline-formula> within a homogeneity composition range of MX<sub>x</sub> at any T although there is no rigorous first-principle-based justification for this a priori assumption. Further, statistical thermodynamic parameter values for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x15.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x16.png" xlink:type="simple"/></inline-formula> evaluated as such yielded enthalpy values comparable to those determined by the conventional thermodynamics for Cr<sub>2</sub>N [<xref ref-type="bibr" rid="scirp.74465-ref3">3</xref>] as well as for several hydrides [<xref ref-type="bibr" rid="scirp.74465-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref18">18</xref>] . Hence, the atomic interaction parameter values evaluated as such by statistical thermodynamics must be considered realistic as well as rational.</p><p>Besides analysis for pure M, analysis was made also for substitutional alloy with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x17.png" xlink:type="simple"/></inline-formula> consisting of two alloying constituents, A and B [<xref ref-type="bibr" rid="scirp.74465-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref24">24</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref35">35</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref36">36</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref38">38</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref40">40</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref42">42</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] as well as for ternary alloy MZ<sub>z</sub>X<sub>x</sub> containing another interstitial constituent Z besides X in which affinity of Z to M was stronger than that of X to M [<xref ref-type="bibr" rid="scirp.74465-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref32">32</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref34">34</xref>] .</p><p>In the early stage of this line of work to characterize nature of atomistic interaction in interstitial non-stoichiometric compound MX<sub>x</sub> [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] - [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] , attention was not paid explicitly on engineering significance of the parameter values evaluated by the statistical thermodynamic analysis. However, after the analysis was made to evaluate interaction parameters for H absorption behaviours for Va-group metal-based alloy membranes [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] , it occurred to the author that it might be of pragmatic convenience if the correlation was established between the estimated values of the interaction parameters by statistical thermodynamic analysis and the reported H permeation performance for the Va-group metal-based alloy membrane materials. This led the author to summarize somewhat speculative paper [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] soon after [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] . The background idea for this attempt of correlating the statistical thermodynamic parameter values evaluated for Va-group metal-based alloy membrane to the H permeation performance of the alloy membrane was to screen promising ones from candidate Va-group metal-based alloys so that the number of H permeation experiments could be minimized. H permeation experiment is time-consuming and the results are dependent on setting of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x18.png" xlink:type="simple"/></inline-formula> on the inlet side and that on the outlet side.</p><p>This special issue of Journal of Modern Physics bears title “Engineering Thermal Physics” with “statistical thermodynamics” being included as one of the possible fields of concern. Thus, the author decided to summarize this manuscript to review comprehensively the engineering significances of the interaction parameters estimated by statistical thermodynamics reported in the published works during the last four decades [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] - [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] .</p><p>As the main purpose of this manuscript is to demonstrate potential usefulness of evaluated atomic interaction parameters for MX<sub>x</sub> by statistical thermodynamics for advanced alloy design, PTC data sources used in the analyses are not cited as the References. Statistical thermodynamic analysis procedures for interstitial non-stoichiometric compound MX<sub>x</sub> shall be reviewed in the next Chapter although they might be referred to elsewhere [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] as the statistical thermodynamic analysis procedure, unlike mathematically well-defined conventional thermodynamic analysis procedure, is not yet widely accepted as a standard analysis tool among materials researchers.</p><p>Among literatures cited in References section of this paper, [<xref ref-type="bibr" rid="scirp.74465-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref25">25</xref>] and [<xref ref-type="bibr" rid="scirp.74465-ref28">28</xref>] were works in which results of statistical thermodynamic analysis were made use of for interpretation of the discussed matters rather than works of statistical thermodynamic analysis itself and [<xref ref-type="bibr" rid="scirp.74465-ref41">41</xref>] was a preparative work to convert the equilibrium data format reported for Fe-Cr-P system by the original authors of the experimental work to a format adequate for straightforward statistical thermodynamic analysis that was published eventually as [<xref ref-type="bibr" rid="scirp.74465-ref42">42</xref>] .</p></sec><sec id="s2"><title>2. Statistical Thermodynamic Analysis Procedure</title><sec id="s2_1"><title>2.1. Fundamental Equations</title><p>Generalized fundamental formulae proposed for this line of analysis of interstitial non-stoichiometric condensed phase MX<sub>x</sub> are as follows.</p><disp-formula id="scirp.74465-formula1096"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x19.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1097"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x20.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1098"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x21.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1099"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x22.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1100"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x23.png"  xlink:type="simple"/></disp-formula><p>Symbols used in the above formulae are classified as follows:</p><p></p><p>R: universal gas constant (=8.31451 J・mol<sup>−1</sup>・K<sup>−1</sup>),</p><p>h: Planck constant (=6.6260755 &#215; 10<sup>−34</sup> J・s),</p><p>k: Boltzmann constant (=1.380658 &#215; 10<sup>−23</sup> J・K<sup>−1</sup>),</p><p></p><p>m<sub>X</sub>: mass of X atom,</p><p>ρ: nuclear spin weight,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x24.png" xlink:type="simple"/></inline-formula>: characteristic temperature for rotation of X<sub>2</sub>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x25.png" xlink:type="simple"/></inline-formula>: characteristic temperature for vibration of X<sub>2</sub>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x26.png" xlink:type="simple"/></inline-formula>: electronic state of normal state of X<sub>2</sub> molecule,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x27.png" xlink:type="simple"/></inline-formula>: dissociation energy of X<sub>2</sub> molecule per mole,</p><p>β: factor determined from crystal structure consideration,</p><p>θ<sub>0</sub>: geometrically available number of interstitial site per M in MX<sub>x</sub>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x28.png" xlink:type="simple"/></inline-formula>: statistical weight of tightly bound electrons around X in MX<sub>x</sub>,</p><p>ν: vibrational frequency of X atom in MX<sub>x</sub> lattice,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x29.png" xlink:type="simple"/></inline-formula>: distribution function,</p><p></p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x30.png" xlink:type="simple"/></inline-formula>: equilibrium pressure of ideal gas X<sub>2</sub>,</p><p>T: absolute temperature (K),</p><p>x: composition (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x31.png" xlink:type="simple"/></inline-formula>atom ratio) in MX<sub>x</sub>,</p><p>n<sub>X</sub>: number of X atoms in MX<sub>x</sub>,</p><p>n<sub>M</sub>: number of M atoms in MX<sub>x</sub>,</p><p></p><p>Q: degree of stabilisation of X atom in MX<sub>x</sub> lattice with reference to isolated X and M atoms in vacuum,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x32.png" xlink:type="simple"/></inline-formula>: interaction energy between i and j atoms in MX<sub>x</sub> lattice,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x33.png" xlink:type="simple"/></inline-formula>: lattice energy,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x34.png" xlink:type="simple"/></inline-formula>: partition function of X atom in MX<sub>x</sub>,</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x35.png" xlink:type="simple"/></inline-formula>: partition function of M atom in MX<sub>x</sub>,</p><p>K &amp; g: parameters determined by Equations (1) &amp; (2), from the experimental PTC data for an assigned value of θ,</p><p></p><p>θ: number of the interstitial sites per M atom available for occupation by X atoms in MX<sub>x</sub>,</p><p></p><p>Z: extent of blocking of interstitial sites by X in<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x36.png" xlink:type="simple"/></inline-formula>; that is, when one interstitial site in MX<sub>x</sub> is occupied by an X atom, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x37.png" xlink:type="simple"/></inline-formula>neighbouring interstitial sites are blocked from occupation by other X atoms.</p><p>For example, in case that X atoms in MX<sub>x</sub> occupy octahedral interstitial sites (O-sites) expression for Q in close packed lattices like fcc (face centred cubic) and hcp (hexagonal close packed) is simply,</p><disp-formula id="scirp.74465-formula1101"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x38.png"  xlink:type="simple"/></disp-formula><p>but that for bcc (body centred cubic) lattice is expressed as</p><disp-formula id="scirp.74465-formula1102"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x39.png"  xlink:type="simple"/></disp-formula><p>taking into account second nearest neighbour interactions, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x40.png" xlink:type="simple"/></inline-formula>and</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x41.png" xlink:type="simple"/></inline-formula>, besides nearest neighbour <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x42.png" xlink:type="simple"/></inline-formula> interaction <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x43.png" xlink:type="simple"/></inline-formula> due to openness of the atom packing in the bcc crystal lattice [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref18">18</xref>] .</p><p>On the other hand, geometrical factor β to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x44.png" xlink:type="simple"/></inline-formula> in Equation (1) might be non-integral number. For example, β is 4/3 if X atoms are distributed over O-sites in bcc lattice [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref18">18</xref>] .</p><p>Value of θ to fulfill the a priori assumption of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x45.png" xlink:type="simple"/></inline-formula> within a homogeneity range of MX<sub>x</sub> at arbitrary T is usually close to the solubility limit of X in the MX<sub>x</sub>. For example, in the statistical thermodynamic analysis of hypo-stoichiometric Cr<sub>2</sub>N phase, θ was chosen to be 0.50 to fulfill the condition of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x46.png" xlink:type="simple"/></inline-formula> over the homogeneity composition range of Cr<sub>2</sub>N [<xref ref-type="bibr" rid="scirp.74465-ref3">3</xref>] . When θ was chosen to be 1 (=θ<sub>0</sub> for O-site occupation of N in the hcp lattice), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x46.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x47.png" xlink:type="simple"/></inline-formula>varied with x showing trend of increasing positive (repulsive)</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x48.png" xlink:type="simple"/></inline-formula>with increasing x. If such variation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x49.png" xlink:type="simple"/></inline-formula> takes place in MX<sub>x</sub>, it is more natural to accept phase change to occur rather than to hold the same crystal lattice structure [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] .</p></sec><sec id="s2_2"><title>2.2. Analysis Procedure</title><p>At the onset of the analysis, isothermal A vs. x plots must be prepared from available isothermal PC relationship at arbitrary T using Equation (1) by varying θ. As understood from Equation (1), slope of isothermal A vs. x plot would become proportional to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x50.png" xlink:type="simple"/></inline-formula>. To fulfill the a priori assumption of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x51.png" xlink:type="simple"/></inline-formula> within homogeneity composition range of MX<sub>x</sub> at arbitrary T, θ yielding linear A vs. x relationship over entire homogeneity composition range of MX<sub>x</sub> must be chosen for the subsequent calculations.</p><p>Then, from the intercept g(T) calculated using Equation (1), K(T) vs. T relationship must be drawn using Equation (2). Term Q on the right hand side in Equation (2) refers to extent of stabilization of atom X in the MX<sub>x</sub> lattice due to formation of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x52.png" xlink:type="simple"/></inline-formula> bonds in the MX<sub>x</sub> lattice while the coefficient</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x53.png" xlink:type="simple"/></inline-formula>to T refers to electronic contribution to entropy term in thermodynamic sense. In fact, partition function <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x54.png" xlink:type="simple"/></inline-formula> of X atom in the MX<sub>x</sub> lattice is a T-dependent function as represented by Equation (4) but, as the T range of statistical thermodynamic analysis for MX<sub>x</sub> is typically no wider than 500 K, it has been a common practice to approximate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x55.png" xlink:type="simple"/></inline-formula> as a T-independent constant term [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] - [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] .</p><p>For convenience of the readers, flow chart of the calculation procedure is presented below as <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>As represented by Equation (5), term <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula> refers to the net extent of stabilization of X atom in the MX<sub>x</sub> lattice, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x57.png" xlink:type="simple"/></inline-formula>, taking into account the contribution of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x58.png" xlink:type="simple"/></inline-formula> interaction besides Q which represents contribution of the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x59.png" xlink:type="simple"/></inline-formula> interaction alone where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x60.png" xlink:type="simple"/></inline-formula> refers to lattice energy of compound MX<sub>x</sub> calculated taking into account all nearest neighbour pairwise atomic interactions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x58.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x61.png" xlink:type="simple"/></inline-formula> for all combinations of i and j.</p><p>For pragmatic convenience of calculating K(T) using Equation (2),</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x62.png" xlink:type="simple"/></inline-formula>values for X = H and N are presented in tabulated form in [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] and [<xref ref-type="bibr" rid="scirp.74465-ref37">37</xref>] at 100 K interval from 0 K up to 3000 K so that</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x63.png" xlink:type="simple"/></inline-formula>value at arbitrary T is calculated readily by interpolation although values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x64.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x65.png" xlink:type="simple"/></inline-formula> were taken from JANAF Thermochemical Tables [<xref ref-type="bibr" rid="scirp.74465-ref49">49</xref>] or NIST-JANAF Thermochemical Tables [<xref ref-type="bibr" rid="scirp.74465-ref50">50</xref>] .</p></sec></sec><sec id="s3"><title>3. Some Insights Drawn from Statistical Thermodynamic Analysis Results for Interstitial Non-Stoichiometric Compounds</title><sec id="s3_1"><title>3.1. Stability of X in FeX<sub>x</sub> Lattice</title><p>As might be understood from expressions for fundamental equations reviewed in 2.1., reference state of energy in the statistical thermodynamic analysis is each constituent atom in infinite separation in vacuum whereas the reference state of constituent in conventional thermodynamic analysis is the pure substance in standard state. That is, by conventional thermodynamic analysis, enthalpy of formation of MX<sub>x</sub> from M and X<sub>2</sub> represents the difference in energy between the reaction product MX<sub>x</sub> and the reactants, M and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x66.png" xlink:type="simple"/></inline-formula>, rather than <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x67.png" xlink:type="simple"/></inline-formula> evaluated by the statistical thermodynamic analysis. This makes straightforward comparison of extent of stabilization of different X atoms in a</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title>Flow chart of the statistical thermodynamic analysis procedure accepting a priori assumption of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x69.png" xlink:type="simple"/></inline-formula> within homogeneity composition range of MX<sub>x</sub> at arbitrary temperature T</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x68.png"/></fig><p>given M lattice difficult through conventional thermodynamic analysis. In contrast, statistical thermodynamic analysis results allow us to compare straightforwardly the relative stability of different X’s in a given M as seen in <xref ref-type="table" rid="table">Table </xref>1 for M = Fe and X = H, C, N, P and S [<xref ref-type="bibr" rid="scirp.74465-ref20">20</xref>] .</p><p>The more stable the X in Fe lattice the more negative would become <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x70.png" xlink:type="simple"/></inline-formula> in FeX<sub>x</sub> lattice. That is, according to <xref ref-type="table" rid="table">Table </xref>1, the stability of X in Fe lattice would decrease in the order of</p><disp-formula id="scirp.74465-formula1103"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x71.png"  xlink:type="simple"/></disp-formula><p>implying that C is the most stable and H is the least stable in Fe lattice.</p><p>Further, it is notice in <xref ref-type="table" rid="table">Table </xref>1 that, for given X, stability in Fe lattice would vary depending on the lattice structure of Fe</p><disp-formula id="scirp.74465-formula1104"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x72.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1105"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x73.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1106"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x74.png"  xlink:type="simple"/></disp-formula><p>implying that the most stable state of C in Fe is realized in molten state, that of N in γ phase and that of H in α phase.</p><p>In <xref ref-type="table" rid="table">Table </xref>1, θ value of some MX<sub>x</sub> is not specified uniquely. This is due to inherent difficulty of determining exactly the value of θ for statistical thermodynamic</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table">Table </xref>1</label><caption><title> Estimated values of Q in miscellaneous FeX<sub>x</sub> (reproduced from <xref ref-type="table" rid="table">Table </xref>1 in [<xref ref-type="bibr" rid="scirp.74465-ref20">20</xref>] )</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >Compound</th><th align="center" valign="middle" >Range of T</th><th align="center" valign="middle"  rowspan="2"  >θ</th><th align="center" valign="middle" >Q<sup>b</sup></th></tr></thead><tr><td align="center" valign="middle" >[K]</td><td align="center" valign="middle" >[kJ・mol<sup>−1</sup>]</td></tr><tr><td align="center" valign="middle" >α-FeH<sub>x</sub> (bcc)</td><td align="center" valign="middle" >&lt;1175</td><td align="center" valign="middle" >&gt;0.01</td><td align="center" valign="middle" >−171</td></tr><tr><td align="center" valign="middle" >γ-FeH<sub>x</sub> (fcc)</td><td align="center" valign="middle" >1185 - 1590</td><td align="center" valign="middle" >(0.50)<sup>a</sup></td><td align="center" valign="middle" >−138</td></tr><tr><td align="center" valign="middle" >δ-FeH<sub>x</sub> (bcc)</td><td align="center" valign="middle" >1665 - 1715</td><td align="center" valign="middle" >(0.50)<sup>a</sup></td><td align="center" valign="middle" >−100</td></tr><tr><td align="center" valign="middle" >α-FeC<sub>x</sub> (bcc)</td><td align="center" valign="middle" >&lt;1000</td><td align="center" valign="middle" >&gt;0.10</td><td align="center" valign="middle" >−648</td></tr><tr><td align="center" valign="middle" >α-FeC<sub>x</sub> (bcc)</td><td align="center" valign="middle" >1025 - 1150</td><td align="center" valign="middle" >&gt;0.10</td><td align="center" valign="middle" >−613</td></tr><tr><td align="center" valign="middle" >γ-FeC<sub>x</sub> (fcc)</td><td align="center" valign="middle" >1175 - 1575</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >−679</td></tr><tr><td align="center" valign="middle" >FeC<sub>x</sub> (molten)</td><td align="center" valign="middle" >1550 - 1775</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >−699</td></tr><tr><td align="center" valign="middle" >α-FeN<sub>x</sub> (bcc)</td><td align="center" valign="middle" >&lt;1115</td><td align="center" valign="middle" >&gt;0.05</td><td align="center" valign="middle" >−420</td></tr><tr><td align="center" valign="middle" >γ-FeN<sub>x</sub> (fcc)</td><td align="center" valign="middle" >1250 - 1625</td><td align="center" valign="middle" >(0.50)<sup>a</sup></td><td align="center" valign="middle" >−455</td></tr><tr><td align="center" valign="middle" >δ-FeN<sub>x</sub> (bcc)</td><td align="center" valign="middle" >1675 - 1715</td><td align="center" valign="middle" >(0.50)<sup>a</sup></td><td align="center" valign="middle" >−352</td></tr><tr><td align="center" valign="middle" >FeN<sub>x</sub> (molten)</td><td align="center" valign="middle" >1850 - 2000</td><td align="center" valign="middle" >&gt;0.10</td><td align="center" valign="middle" >−427</td></tr><tr><td align="center" valign="middle" >FeP<sub>x</sub> (molten)</td><td align="center" valign="middle" >1475 - 1775</td><td align="center" valign="middle" >0.50</td><td align="center" valign="middle" >−347</td></tr><tr><td align="center" valign="middle" >FeS<sub>x</sub> (molten)</td><td align="center" valign="middle" >1775 - 1875</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >−307</td></tr></tbody></table></table-wrap><p>a. Value of θ used for convenience on calculating Q value for the very dilute interstitial solution. b. Q corresponds to partial molar enthalpy of solution h(X) of X into Fe. Some h(X) values reported by McLellan and co-workers (da Silva, J. R. G and McLellan, R. B. (1976) The Solubility of Hydrogen in Super-pure-ron Single Crystals. J. Less Coomon Met., 50, 1 - 5.; McLellan, R. B. and Farraro, R. J. Thermodynamics of the Iron-Nitrogen System. (1980) Acta. Metall., 28, 417-422.) were in good accord with the corresponding values of Q. h(H)<sup>α</sup> = −177 kJ・mol<sup>−1</sup>: Q(H)<sup>α</sup> = −171 kJ・mol<sup>−1</sup>, h(C)<sup>α</sup> = −603 kJ・mol<sup>−1</sup>: Q(C)<sup>α</sup>(T &gt; T<sub>C</sub>) = −613 kJ・mol<sup>−1</sup>, Q(C)<sup>α</sup>(T &lt; T<sub>C</sub>) = −648 kJ・mol<sup>−1</sup>, h(C)<sup>γ</sup> = −650 kJ・mol<sup>−1</sup>: Q(C)<sup>γ</sup> = −699 kJ・mol<sup>−1</sup>, h(N)<sup>α</sup> = −424 kJ・mol<sup>−1</sup>: Q(N)<sup>α</sup> = −420 kJ・mol<sup>−1</sup>, h(N)<sup>γ</sup> = −460 kJ・mol<sup>−1</sup>: Q(N)<sup>γ</sup> = −455 kJ・mol<sup>−1</sup>, where T<sub>C</sub> refers to Curie temperature 1043 K for Fe.</p><p>analysis in very dilute interstitial solution under certain circumstances as discussed in some detail in [<xref ref-type="bibr" rid="scirp.74465-ref15">15</xref>] .</p><p>First cases of statistical thermodynamic analysis for very dilute interstitial solutions was made in [<xref ref-type="bibr" rid="scirp.74465-ref11">11</xref>] in which a priori condition of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x75.png" xlink:type="simple"/></inline-formula> was set to fulfill the condition</p><disp-formula id="scirp.74465-formula1107"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x76.png"  xlink:type="simple"/></disp-formula><p>noting the reality that, in the very dilute interstitial compound, there must be no neighbouring interstitial atom around any interstitial atom.</p><p>However, when solutions of H, C and N in α-Fe was investigated in terms of statistical thermodynamics, unambiguous specification of θ to fulfill condition (12) was difficult but, instead, when θ value was taken to be greater than certain threshold value, estimated value of Q converged to a constant level whereas, in the range of θ smaller than the threshold level, estimated value of Q showed steady variation with varying θ (cf. <xref ref-type="fig" rid="fig2">Figure 2</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref15">15</xref>] ). On account of this situation, unique specification of θ was given up for some very dilute interstitial compounds and, as a compromising solution, θ value which must have been greater than the threshold level was used for the analysis because, by so doing, realistic value for Q was evaluated as discussed in [<xref ref-type="bibr" rid="scirp.74465-ref15">15</xref>] although value of the product Zf<sub>X</sub> varied as a function of θ in the range of θ where Q value became constant with θ.</p></sec><sec id="s3_2"><title>3.2. Atom Clustering in Fe<sub>1−y</sub>M<sub>y</sub>X<sub>x</sub> around X Atom</title><p>During the course of statistical thermodynamic analysis of PTC relationships reported for N solution in molten Fe<sub>1−y</sub>M<sub>y</sub> in which affinity of M to N is stronger than that of Fe to N, it was concluded that certain types of atom clustering might develop around interstitial N atom [<xref ref-type="bibr" rid="scirp.74465-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref24">24</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref26">26</xref>] . This aspect shall be reviewed in the following.</p><p>As always in this line of statistical thermodynamic analysis, θ parameter values on analysis of molten Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> for varying y were determined accepting an a priori assumption of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x77.png" xlink:type="simple"/></inline-formula> over homogeneity composition of Fe<sub>1−y</sub>CryNx as reproduced in <xref ref-type="fig" rid="fig2">Figure 2</xref> and, by the statistical thermodynamic</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title>Relationship between θ and y in molten Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> to fulfill the a priori condition of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x79.png" xlink:type="simple"/></inline-formula> over homogeneity composition range at arbitrary T (reproduced from <xref ref-type="fig" rid="fig3">Figure 3</xref>.57 in [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] or <xref ref-type="fig" rid="fig4">Figure 4</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref24">24</xref>] )</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x78.png"/></fig><p>analysis done with the θ values determined as such, values of R ln Zf<sub>N</sub>(Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub>) (a) and Q(Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub>) (b) were obtained as a function of y as reproduced in <xref ref-type="fig" rid="fig3">Figure 3</xref>. In spite of somewhat peculiar variation pattern of θ with y (<xref ref-type="fig" rid="fig2">Figure 2</xref>), variation patterns of Q and R ln Zf<sub>N</sub> with respect to y looked quite “regular” (<xref ref-type="fig" rid="fig3">Figure 3</xref>). In this analysis, molten Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> at temperatures close to liquidus temperature above Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> solid phase possessing fcc structure was assumed to hold fcc structure. In the range of low y not exceeding 0.2, θ varied following</p><disp-formula id="scirp.74465-formula1108"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x80.png"  xlink:type="simple"/></disp-formula><p>For this range of θ (&lt;0.2), the interpretation was quite simple. That is, N atom in an O site was assumed to become surrounded by one Cr atom and 5 Fe atoms (1 Cr/5 Fe cluster or Cr-N dipole) as depicted in <xref ref-type="fig" rid="fig4">Figure 4</xref>(a). Q values determined</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Estimated values of R ln Zf<sub>N</sub> [J・K<sup>−1</sup>・mol<sup>−1</sup>] (a) and Q [kJ・mol<sup>−1</sup>] (b) for molten Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> plotted as a function of y. In <xref ref-type="fig" rid="fig2">Figure 2</xref>(b), positions of values of Q estimated from proportional sum of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x82.png" xlink:type="simple"/></inline-formula> = −72 [kJ・mol<sup>−1</sup>] and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x83.png" xlink:type="simple"/></inline-formula> = −93 [kJ・mol<sup>−1</sup>] at various satom ratios of Cr to Fe are given by horizontal dotted line (reproduced from <xref ref-type="fig" rid="fig3">Figure 3</xref>.58 in [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] or <xref ref-type="fig" rid="fig5">Figure 5</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref24">24</xref>] )</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x81.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title>Possible atom clusters formed in fcc Fe<sub>1−y</sub>Cr<sub>y</sub>N<sub>x</sub> lattice in which affinity of M to N is stronger than that of Fe to N. (a) 1 M/5 Fe cluster (composed of one M atom and five Fe atoms around N); θ = y, (b) 2 M/4 Fe cluster; θ = y/2 and (c) 4 M/2 Fe cluster, θ = y/4 (reproduced from <xref ref-type="fig" rid="fig3">Figure 3</xref>.59 in [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] or <xref ref-type="fig" rid="fig3">Figure 3</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref26">26</xref>] )</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x84.png"/></fig><p>in the range of y smaller than 0.20 was consant with y being represented approxi- mately by</p><disp-formula id="scirp.74465-formula1109"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x85.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x86.png" xlink:type="simple"/></inline-formula> refers to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x87.png" xlink:type="simple"/></inline-formula> interaction energy (≈−93 [kJ・mol<sup>−1</sup>]) in molten CrN<sub>x</sub> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x87.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x88.png" xlink:type="simple"/></inline-formula> N-Fe interaction (≈−72 [kJ・mol<sup>−1</sup>]) in molten FeN<sub>x</sub> [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref24">24</xref>] .</p><p>On the other hand, it was felt difficult to appreciate rationally the variation pattern of θ with y in the range of y higher than 0.4 at first glance. However, as seen in <xref ref-type="fig" rid="fig3">Figure 3</xref>, Q values determined in the range of 0.4 ≤ y &lt; 1 was consant with y being represented approximately by</p><disp-formula id="scirp.74465-formula1110"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x89.png"  xlink:type="simple"/></disp-formula><p>implying formation of 4 Cr/2 Fe cluster as depicted in <xref ref-type="fig" rid="fig4">Figure 4</xref>(c).</p><p>Detected deviation of θ vs. y relationship from the one represented by</p><disp-formula id="scirp.74465-formula1111"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x90.png"  xlink:type="simple"/></disp-formula><p>in <xref ref-type="fig" rid="fig2">Figure 2</xref> was interpreted to be the consequence of Guinier-Preston zone type planar extensiton of 4 Cr/2 Fe clusters as detected in <xref ref-type="fig" rid="fig4">Figure 4</xref>(c).</p><p>To explain why θ vs. y relationship in range of y between 0.4 and 0.9 in <xref ref-type="fig" rid="fig2">Figure 2</xref> deviated from the relationsip defined by Equation (16), model Guinier-Preston zone type planar extensions of 4 M/2 Fe clusters for a fixed numnber 12 of M atoms leading to different values of θ are depicted in <xref ref-type="fig" rid="fig5">Figure 5</xref>. As seen in <xref ref-type="fig" rid="fig5">Figure 5</xref>(b) and <xref ref-type="fig" rid="fig5">Figure 5</xref>(c), increased degree of planar extensiton would yield higher value of θ than the one anticipated from Equation (16) defined for the isolated 4 M/2 Fe clusters depcited in <xref ref-type="fig" rid="fig5">Figure 5</xref>(a).</p><p>It is intriguing to note that no evidence of existence of 2 M/4 Fe cluster as depicted in <xref ref-type="fig" rid="fig4">Figure 4</xref>(b) was detected for A<sub>1−y</sub>B<sub>y</sub>X<sub>x</sub> type interstitial non-stopichio- metric compounds analyzed so far.</p></sec><sec id="s3_3"><title>3.3. Design Guideline for H Permeable Alloy Membrane</title><p>Yukawa and collaborators at Nagoya University [<xref ref-type="bibr" rid="scirp.74465-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref52">52</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref53">53</xref>] experimentally</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title>Some possible ways of planar extention of the 4 M/2 Fe cluster depicted in <xref ref-type="fig" rid="fig3">Figure 3</xref>(c) over the (002) plnae of fcc lattice leading to different values of θ with a fixed number of 12 M atoms. (a) isolated clusters, θ = y/4, (b) planar extensiton leading to θ = (5/12)y and (c) planar extenstion leading to θ = (6/12)y = y/2 (reproduced from <xref ref-type="fig" rid="fig3">Figure 3</xref>.60 in [<xref ref-type="bibr" rid="scirp.74465-ref2">2</xref>] or <xref ref-type="fig" rid="fig4">Figure 4</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref26">26</xref>] )</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x91.png"/></fig><p>investigated H permeation behaviors as well as H absorption behaviors for Va-group metal-based alloy membranes. The author [<xref ref-type="bibr" rid="scirp.74465-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref47">47</xref>] analyzed the reported PCT relationships by Yukawa and collaborators [<xref ref-type="bibr" rid="scirp.74465-ref49">49</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref50">50</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref51">51</xref>] and obtained values for parameters, Q and R ln Zf<sub>H</sub>, as summarized in <xref ref-type="table" rid="table">Table </xref>2.</p><p>According to Yukawa and co-workers, Va-group metal-based alloys identified as favuorable H permeation membrane includes V<sub>0.95</sub>Fe<sub>0.05</sub> [<xref ref-type="bibr" rid="scirp.74465-ref49">49</xref>] , Nb<sub>0.95</sub>Ru<sub>0.05</sub> and Nb<sub>0.95</sub>W<sub>0.05</sub> [<xref ref-type="bibr" rid="scirp.74465-ref50">50</xref>] as well as Ta<sub>0.95</sub>W<sub>0.05</sub> [<xref ref-type="bibr" rid="scirp.74465-ref51">51</xref>] . Looking at values of θ and Q for these A<sub>1−y</sub>M<sub>y</sub> type alloys containing Va-group metal (represented by A) in <xref ref-type="table" rid="table">Table </xref>2, it is noticed that θ was smaller and Q was more negative in this group of alloys than those in pure Va-group metal A except Ta<sub>0.95</sub>W<sub>0.05</sub>. Thus, it was proposed [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] to use the simultaneous fulfillment of conditions</p><disp-formula id="scirp.74465-formula1112"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x92.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1113"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x93.png"  xlink:type="simple"/></disp-formula><p>for screening of H permeation alloy membrane from among the candidate alloys</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table">Table </xref>2</label><caption><title> Available statistical thermodynamic interaction parameter for bcc A<sub>1−y</sub>M<sub>y</sub>H<sub>x</sub> that showed suppressed H solubility compared to that in bcc AH<sub>x</sub> where A refers to Va-group metals (V, Nb or Ta) (reproduced from <xref ref-type="table" rid="table">Table </xref>1 in [<xref ref-type="bibr" rid="scirp.74465-ref48">48</xref>] )</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >bcc A<sub>1−y</sub>M<sub>y</sub>H<sub>x</sub></th><th align="center" valign="middle"  rowspan="2"  >θ</th><th align="center" valign="middle" >Q<sup>a</sup></th><th align="center" valign="middle" >R ln Zf<sub>H</sub></th></tr></thead><tr><td align="center" valign="middle" >[kJ・mol<sup>−1</sup>]</td><td align="center" valign="middle" >[J・K<sup>−1</sup>・mol<sup>−1</sup>]</td></tr><tr><td align="center" valign="middle" >VH<sub>x</sub></td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >−223.6</td><td align="center" valign="middle" >64.7</td></tr><tr><td align="center" valign="middle" >V<sub>0.96</sub>Cr<sub>0.04</sub>Hx</td><td align="center" valign="middle" >0.525</td><td align="center" valign="middle" >−220.0</td><td align="center" valign="middle" >26.9</td></tr><tr><td align="center" valign="middle" >V<sub>0.916</sub>Cr<sub>0.084</sub>Hx</td><td align="center" valign="middle" >0.475</td><td align="center" valign="middle" >−207.2</td><td align="center" valign="middle" >54.5</td></tr><tr><td align="center" valign="middle" >V<sub>0.949</sub>Mo<sub>0.051</sub>Hx</td><td align="center" valign="middle" >0.525</td><td align="center" valign="middle" >−207.3</td><td align="center" valign="middle" >37.5</td></tr><tr><td align="center" valign="middle" >V<sub>0.95</sub>Fe<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >−229.4</td><td align="center" valign="middle" >23.7</td></tr><tr><td align="center" valign="middle" >V<sub>0.948</sub>Co<sub>0.052</sub>Hx</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >−230.1</td><td align="center" valign="middle" >21.5</td></tr><tr><td align="center" valign="middle" >NbH<sub>x</sub></td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >−229.5</td><td align="center" valign="middle" >61.7</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Ru<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >−221.8</td><td align="center" valign="middle" >41.2</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>W<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.725</td><td align="center" valign="middle" >−243.1</td><td align="center" valign="middle" >14.1</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.90</sub>Mo<sub>010</sub>Hx</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >−225.5</td><td align="center" valign="middle" >65.4</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.80</sub>Mo<sub>0.20</sub>Hx</td><td align="center" valign="middle" >0.30</td><td align="center" valign="middle" >−228.2</td><td align="center" valign="middle" >61.3</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.70</sub>Mo<sub>0.30</sub>Hx</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >−220.8</td><td align="center" valign="middle" >67.7</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Al<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >−225.8</td><td align="center" valign="middle" >36.9</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Cu<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >−223.5</td><td align="center" valign="middle" >41.2</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Sn<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >−231.8</td><td align="center" valign="middle" >30.6</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Ni<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >−219.2</td><td align="center" valign="middle" >45.0</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.95</sub>Pd<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.60</td><td align="center" valign="middle" >−231.8</td><td align="center" valign="middle" >26.1</td></tr><tr><td align="center" valign="middle" >Nb<sub>0.90</sub>Pd<sub>0.10</sub>Hx</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >−213.9</td><td align="center" valign="middle" >45.5</td></tr><tr><td align="center" valign="middle" >TaH<sub>x</sub></td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >−229.4</td><td align="center" valign="middle" >62.4</td></tr><tr><td align="center" valign="middle" >Ta<sub>0.95</sub>W<sub>0.05</sub>Hx</td><td align="center" valign="middle" >0.55</td><td align="center" valign="middle" >−228.6</td><td align="center" valign="middle" >32.1</td></tr></tbody></table></table-wrap><p>a. Q values of θ for A<sub>1−y</sub>M<sub>y</sub>H<sub>x</sub> that were evaluated to be more negative than that for AH<sub>x</sub> are displayed with bold letter.</p><p>based on Va-group metal.</p><p>On H permeation process, H<sub>2</sub> gas pressure p(H<sub>2</sub>)<sup>in</sup> on the inlet side of the membrane is set higher than p(H<sub>2</sub>)<sup>out</sup> on the outlet side. On the inlet side of the membrane, adsorbed H<sub>2</sub> gas over the membrane surface must be subjected to dissociation into adsorbed monatomic H atoms before being absorbed into A<sub>1−y</sub>M<sub>y</sub> alloy lattice</p><disp-formula id="scirp.74465-formula1114"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x94.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.74465-formula1115"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-7502999x95.png"  xlink:type="simple"/></disp-formula><p>Then, by concentration gradient along the membrane thickness, absorbed H in the A<sub>1−y</sub>M<sub>y</sub> lattice is subjected to diffusion towards the outlet side of the membrane. On the reaction (20) to proceed at the inlet side of the membrane, condition (18) is certainly favourable to suck faster the H atoms into the A<sub>1−y</sub>M<sub>x</sub> lattice from the inlet side surface.</p><p>Then, on release of the transported H atoms through the outlet side surface of the A<sub>1−y</sub>M<sub>y</sub> membrane, successive inverse reactions, (19) and (20) in this order, must proceed to recombine the absorbed monatomic H atoms in the A<sub>1−y</sub>M<sub>y</sub>X<sub>x</sub> alloy lattice to be released in form of diatomic H<sub>2</sub> gas molecules. For this process of H<sub>2</sub> release to take place faster on the outlet side of the membrane surface, condition (17) is considered to be of convenience.</p><p>As such, simultaneous fulfillment of conditions, (17) and (18), was appreciated as rational for the alloy design guideline for Va-group metal-based H permeation membrane although this criterion did not seem to apply to Ta<sub>0.95</sub>W<sub>0.05</sub> alloy.</p><p>Among Va-group metal-based alloys listed in <xref ref-type="table" rid="table">Table </xref>2, V<sub>0.948</sub>Co<sub>0.052</sub>, Nb<sub>0.95</sub>Sn<sub>0.05</sub> and Nb<sub>0.95</sub>Pd<sub>0.05</sub> fulfill the conditions, (17) and (18), simultaneously although the H permeation performance of these alloys remains unknown.</p></sec><sec id="s3_4"><title>3.4. Constant-a(C) Curves in γ-FeC<sub>x</sub> Phase</title><p>On account of pragmatic industrial importance of steel materials, intensive efforts have been invested on characterizing basic phase relationship for Fe-C binary system in equilibrium state. Taking advantage of abundance of equilibrium data for binary Fe-C system with high qualitative precision, statistical thermodynamic analysis for Fe-C system [<xref ref-type="bibr" rid="scirp.74465-ref20">20</xref>] was done choosing experimental data reported by Ban-ya et al. [<xref ref-type="bibr" rid="scirp.74465-ref54">54</xref>] in which chemical activity a(C) of C in equilibrium with γ-FeC<sub>x</sub> was varied widely through control of p(CO)/p(CO<sub>2</sub>) ratio instead of using C in solid state.</p><p>In common experimental equilibrium study of metal carbide, excess graphite (reference state of C) is arranged to co-exist in the synthesized carbide MC<sub>x</sub>. Under such condition, a(C) is fixed to be 1 and, as such, influence of a(C) on x in MC<sub>x</sub> cannot be evaluated.</p><p>From the statistical thermodynamic analysis, values of θ and Q listed for γ-FeC<sub>x</sub> in <xref ref-type="table" rid="table">Table </xref>1 were calculated and constant-a(C) curves as reproduced in <xref ref-type="fig" rid="fig6">Figure 6</xref> were drawn [<xref ref-type="bibr" rid="scirp.74465-ref20">20</xref>] . This presentation of <xref ref-type="fig" rid="fig6">Figure 6</xref> might be of no practical industrial importance but must be of fundamental significance towards profound</p><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title>Binary Fe-C equilibrium phase diagram compiled by Hansen and Anderko &lt;7&gt; with the estimated constant-a(C) curves and some available experimental results &lt;4&gt;, &lt;5&gt;, &lt;8&gt;, &lt;9&gt; (reproduced from <xref ref-type="fig" rid="fig1">Figure 1</xref> in [<xref ref-type="bibr" rid="scirp.74465-ref20">20</xref>] ). &lt;4&gt; Ban-ya, S, Elliott, J. F. and Chipman, J. (1969) Activity of Carbon in Fe-C Alloys at 1150˚C. Trans. Metall. Soc. AIME, 245, 1199 - 1206; &lt;5&gt; Ban-ya, S., Elliott, J. F. and Chipman, J. (1970) Thermodynamics of Austenitic Fe-C Alloys, Metall. Trans., 1, 1313 - 1320; &lt;7&gt; Hansen, M. and Anderko, K. (1958) Constitution of Binary Alloys, 2nd Ed., McGraw-Hill, New York, Tronto and London; &lt;8&gt; Chipman, J. (1970) Thermodynamics of Liquid Fe-C Solutions, Metall. Trans., 1, 2163 - 2168; &lt;9&gt; Chipman, J. (1972) Thermodynamics and Phase Diagram of the Fe-C System. Metall. Trans., 3, 55-64</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-7502999x96.png"/></fig><p>understanding for inherent nature of interstitial non-stoichiometric compounds like γ-FeC<sub>x</sub>.</p></sec></sec><sec id="s4"><title>4. Conclusions</title><p>A few example cases of estimating properties of interstitial non-stoichiometric compounds with potential industrial applications on the basis of atomic interaction parameters evaluated by statistical thermodynamic analysis were demonstrated in this review article. Looking at the variation pattern of θ parameter value referring to number of available interstitial sites per metal atom M (M might be pure M, A<sub>1−y</sub>B<sub>y</sub> type substitutional alloy or AZ<sub>z</sub> type compound containing another interstitial constituent Z besides interstitial constituent X) with respect to change of y or z, significant insight in atom clustering tendency in the condensed phase might be gained. There are several other materials properties predictable by referring to statistical thermodynamic analysis results including interstitial site occupation information for intermetallic alloys. Interested readers are advised to refer to original papers by the author [<xref ref-type="bibr" rid="scirp.74465-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.74465-ref18">18</xref>] to look into further details.</p><p>The reviewed standardized statistical thermodynamic analysis procedure accepting an a priori assumption of constant <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-7502999x97.png" xlink:type="simple"/></inline-formula> in MX<sub>x</sub> within homogeneity composition range at arbitrary T was proved applicable to interstitial compound holding metallic characteristics but this analysis procedure is not applicable to non-stoichiometric compounds with ionic bonding characteristics like non-stoichiometric oxide.</p><p>Compared with standardized conventional thermodynamic analysis procedure to determine enthalpy, entropy and a few types of free energies through well-established mathematical procedure, statistical thermodynamic analysis is quite tedious demanding reliable PCT data set at least at three different T levels over certain range of p(X<sub>2</sub>) and additional necessity for composing realistic statistical model. This is certainly a drawback of statistical thermodynamic analysis compared with conventional thermodynamics but this feature of statistical thermodynamic approach might be considered as a merit in some sense as the evaluated interaction parameters possess unambiguous physical significance provided that the statistical model used for the analysis is a valid one.</p></sec><sec id="s5"><title>Acknowledgements</title><p>The author would like to thank sincerely Prof. Dr. Masahiro KATSURA who introduced the statistical thermodynamic analysis procedure to the author during the years of apprenticeship at Department of Nuclear Engineering, Faculty of Engineering, Osaka University in 1970s through reading together the classical text book on statistical thermodynamics authored by Fowler and Guggenheim.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.74465-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Fowler, R.H. and Guggenheim, E.A. 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