<?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">JMMCE</journal-id><journal-title-group><journal-title>Journal of Minerals and Materials Characterization and Engineering</journal-title></journal-title-group><issn pub-type="epub">2327-4077</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmmce.2013.14029</article-id><article-id pub-id-type="publisher-id">JMMCE-35103</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Chemistry&amp;Materials Science</subject><subject> Engineering</subject></subj-group></article-categories><title-group><article-title>
 
 
  Analytical Solutions and Computer Simulations of the Evolution of Flat Temperature Profiles in Spherical FRRPP Systems
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>erard</surname><given-names>T. Caneba</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>Mathkar</surname><given-names>A. Alharthi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Chemical Engineering, Michigan Technological University, Houghton, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>caneba@mtu.edu(ETC)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>07</month><year>2013</year></pub-date><volume>01</volume><issue>04</issue><fpage>184</fpage><lpage>191</lpage><history><date date-type="received"><day>April</day>	<month>8,</month>	<year>2013</year></date><date date-type="rev-recd"><day>May</day>	<month>27,</month>	<year>2013</year>	</date><date date-type="accepted"><day>June</day>	<month>14,</month>	<year>2013</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>
 
 
  The free-radical retrograde-precipitation (FRRPP) process was recently brought into the quantitative areas of work, based on the discovery of possibility of flat temperature profiles in spherical reactive domain systems. With an approximate decoupling analysis of the energy equation from the component-balance equations, these flat temperature profiles were found to be either stable or unstable. Moreover, resulting evolution of the flat profiles has been found to be expressed analytically through the so-called exponential Integral function, which has been shown to be quantitatively inaccurate during the early times of the process. This work tries to resolve this inaccuracy problem, by comparing the exponential integral results with polynomial approximation and numerical results. The result is that for the stable sys-tem, the linearized treatment of the evolution of flat temperature profiles is valid at the early 30% - 40% in the tem-perature axis, while the remainder of the evolution curve is well-represented by the application of the exponential integral function. For the unstable system, the only thing that can be generalized is that both linear and cubic polynomial approximations are reasonably accurate at very small times and temperatures close to initial values. 
     
 
</p></abstract><kwd-group><kwd>Flat Temperature Profile; FRRPP; Polymerization; Nonisothermal Reaction; Spherical Reactive Domains; Exponential Integral Function</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>A reactive spherical chain-polymerization particulate system with an exothermic heat of reaction is normally expected to exhibit a parabolic temperature profile, as depicted in <xref ref-type="fig" rid="fig1">Figure 1</xref>. In these systems, the idea of a flat temperature profile is almost unheard of, and potentially beneficial in terms of operational and product uniformity. Also, the analysis of the model equations can become less complicated for these types of systems, because a field dynamics problem can be reduced to the relative simplicity of a lumped-parameter system.</p><p>In recent publications [1,2], it has been conceptually shown that the so-called free-radical retrograde-precipitation polymerization (FRRPP) process can result in flat temperature profiles through a combination of thermodynamic, transport, and reaction-kinetic parameters in the system. This is shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>, wherein the profile starts at a uniform Dimensionless T (or θ in Equation (6)) of 1.0. The temperature profile ends at a steady-state value of Dimensionless T = 1.83 [<xref ref-type="bibr" rid="scirp.35103-ref3">3</xref>]. Note that the dimensionless r in the horizontal axis of <xref ref-type="fig" rid="fig2">Figure 2</xref> is the same as h in Equation (7). This means that the reactive fluid will have h ranging from 0 to 1 only. Values of h between 1 and 2 are rescaled so that they correspond to those of the stagnant fluid boundary layer.</p><p>The prediction of the possibility of the occurrence of flat temperature profiles from FRRPP systems has been advanced from a pseudo-steady-state analysis of the energy balance of a model spherical reacting system undergoing polymerization-induced phase separation [<xref ref-type="bibr" rid="scirp.35103-ref1">1</xref>]. The dimensionless differential energy balance has been shown as</p><disp-formula id="scirp.35103-formula150088"><label>(1)</label><graphic position="anchor" xlink:href="9-2710096\8592cc3f-1867-44ca-9da2-2dd3a23ee9cf.jpg"  xlink:type="simple"/></disp-formula><p>and the dimensionless energy source term Φ is expressed as</p><disp-formula id="scirp.35103-formula150089"><label>(2)</label><graphic position="anchor" xlink:href="9-2710096\6c1a9764-2e7b-40e1-9b6a-b151f7483f32.jpg"  xlink:type="simple"/></disp-formula><p>The dimensionless parameters are related to the following dimensional quantities in the energy balance and phase equilibria equations:</p><disp-formula id="scirp.35103-formula150090"><label>(3)</label><graphic position="anchor" xlink:href="9-2710096\b10c70ff-3325-4a41-8350-4d4b1ce593a4.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150091"><label>(4)</label><graphic position="anchor" xlink:href="9-2710096\5857d22e-b699-4246-9658-dffc279d2acb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150092"><label>(5)</label><graphic position="anchor" xlink:href="9-2710096\8eda6949-be74-4882-b16e-cf6fd457a6fc.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150093"><label>(6)</label><graphic position="anchor" xlink:href="9-2710096\00ec4360-997b-43e7-824e-16264cdd94d7.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150094"><label>(7)</label><graphic position="anchor" xlink:href="9-2710096\971943c2-d9f4-430b-9af4-3b714bb21159.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150095"><label>(8)</label><graphic position="anchor" xlink:href="9-2710096\58bb8297-516b-40b2-b957-aef912033b8b.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150096"><label>(9)</label><graphic position="anchor" xlink:href="9-2710096\46c7e642-d557-4c1b-b6f3-d3a811ac5a92.jpg"  xlink:type="simple"/></disp-formula><p>The phase behavior for the polymer-rich phase was approximated by the linear representation</p><disp-formula id="scirp.35103-formula150097"><label>(10)</label><graphic position="anchor" xlink:href="9-2710096\211b86eb-d0d5-4b0b-bf49-410968453c48.jpg"  xlink:type="simple"/></disp-formula><p>where X<sub>P</sub> is the product of the weight fractions of the monomer and polymer (or just the weight fraction of the polymer if the monomer concentration is the same for both polymer-rich and polymer-lean phases at equilibrium, as the case for the PS-S-Ether system [4,5]. Since Equation (10) provides a mesoscopic-macroscopic relationship between the temperature and monomer composition, it allows the decoupling of the mesocopic-macroscopic analysis of the time evolution behavior of the thermal aspect of the system from compositional aspects, until the details of the kinetics of microphase separation behavior is incorporated in the field equations.</p><p>In order to quantitatively characterize the relatively lower inefficiency of radical maintenance in free-radical polymerization systems, the expression for X<sub>P</sub> in Equation (10) can be modified to include a polymer radical efficiency factor f<sub>P</sub>; thus,</p><disp-formula id="scirp.35103-formula150098"><label>(11)</label><graphic position="anchor" xlink:href="9-2710096\121269fb-fdbc-4948-b67d-843bbe3d98c9.jpg"  xlink:type="simple"/></disp-formula><p>Also, a and b in Equation (10) were proposed to be obtained from experimental data points of phase equilibria experiments. It should be noted that the polymer radical efficiency factor, f<sub>P</sub>, is related to the initiator efficiency, f, in free-radical polymerizations in a relative sense, i.e., for the same monomer, solvent, their concentrations, and operating temperatures, f<sub>P</sub> is relatively high when an initiator with a relatively high f is used. The reason is that initiation is the starting point in time when inefficiencies of radical production take place. The survival of propagated radicals will later depend on the effectiveness of the FRRPP radical trapping mechanism, which should result in f<sub>P</sub> &lt; f. For example, in FRRPP of polystyrene-styrene-ether systems using azobis diisobutylonitrile (AIBN) as initiator, f<sub>P</sub> was found to be in the order of 0.20 [1,4] even though f was known to be around 0.57 [<xref ref-type="bibr" rid="scirp.35103-ref6">6</xref>].</p><p>For the expectation of a flat temperature profile, θ = 1 for η = 0; thus, the dimensionless source term was symbolized as Φ<sub>o</sub> and Equation (2) became</p><disp-formula id="scirp.35103-formula150099"><label>(12)</label><graphic position="anchor" xlink:href="9-2710096\9a29637d-0ff9-4936-a6ec-bf0cf52187ae.jpg"  xlink:type="simple"/></disp-formula><p>Then, a combined dimensionless quantity was introduced to quantitatively characterize strict FRRPP behavior, wherein the reactive polymer-rich domains attained flat temperature profiles. The dimensionless quantity was symbolized by <img src="9-2710096\650be181-50f8-42c8-aafc-13a61ef2e3b2.jpg" /> (pronounced see-enye), and defined as</p><disp-formula id="scirp.35103-formula150100"><label>(13)</label><graphic position="anchor" xlink:href="9-2710096\19b23cb6-9a26-4b63-ad05-26fc45ade2ce.jpg"  xlink:type="simple"/></disp-formula><p>Values of <img src="9-2710096\3a98de83-1600-40b0-8d36-df6039258675.jpg" /> from computational efforts indicated that for the FRRPP process, it should be at least below −1000 for a flat temperature profile [<xref ref-type="bibr" rid="scirp.35103-ref1">1</xref>].</p><p>In the unsteady-state analysis of the FRRPP system, the occurrence of the flat temperature profile from FRRPP systems was reinforced, with additional criteria for stability of steady-state behavior [<xref ref-type="bibr" rid="scirp.35103-ref2">2</xref>]. For a stable steady-state system, it was found that the quantity α &lt; 0 even for an insulated reactive domain system. For a &gt; 0, the reactive system was found to be under control with the possibility of a flat temperature profile through relatively ineffective heat removal from the fluid. With more aggressive heat removal from the fluid, the temperature profile in the reactive solid becomes more of a parabolic one.</p><p>When the monomer concentration drops to low enough values, the reactive system automatically reverts to a stable one, because the value of α automatically becomes a negative number [<xref ref-type="bibr" rid="scirp.35103-ref1">1</xref>]. This happens either locally (due to relatively fast reaction rate compared to diffusion rate, or polymer domain densification [<xref ref-type="bibr" rid="scirp.35103-ref2">2</xref>]) or in the overall reactive system, due to depletion of monomer molecules.</p><p>With assumption of a flat temperature profile, the field energy balance equation was simplified to a mixing-cup ordinary differential equation and later analyzed for its stability characteristics [<xref ref-type="bibr" rid="scirp.35103-ref2">2</xref>]. Results from the field partial differential equation correspond to the reacting sphere with insulated surfaces. An analytical expression for the modified dimensionless temperature (Q) vs dimensionless time (τ) was also obtained for the flat temperature profile reactive spherical domain with insulated boundary surfaces as</p><disp-formula id="scirp.35103-formula150101"><label>(14)</label><graphic position="anchor" xlink:href="9-2710096\73c28d8a-2b02-4910-bf91-040745b150fe.jpg"  xlink:type="simple"/></disp-formula><p>in which the dimensionless time was expressed as</p><disp-formula id="scirp.35103-formula150102"><label>(15)</label><graphic position="anchor" xlink:href="9-2710096\69ee48c7-b032-4d9e-b702-2b06b883f304.jpg"  xlink:type="simple"/></disp-formula><p>and the modified dimensionless temperature (Q),<img src="9-2710096\4597c08a-fce5-45f1-b2a5-3c0c060e8cf5.jpg" />and <img src="9-2710096\da21ddf3-57f1-4e9f-b8a1-e71723c50d72.jpg" /> are obtained as</p><disp-formula id="scirp.35103-formula150103"><label>(16)</label><graphic position="anchor" xlink:href="9-2710096\867b4d66-5da7-4d63-87f2-aab5afc88b86.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150104"><label>(17)</label><graphic position="anchor" xlink:href="9-2710096\a1b35fdd-9a21-4986-bbce-037b921433b2.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150105"><label>(18)</label><graphic position="anchor" xlink:href="9-2710096\b678fcd5-e165-473a-9244-2ec73e5f1185.jpg"  xlink:type="simple"/></disp-formula><p>Note that T<sub>b</sub> is the bulk fluid temperature while T<sub>s</sub> is the reactive particle surface temperature (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>The function, Ei or the Exponential Integral Function [<xref ref-type="bibr" rid="scirp.35103-ref7">7</xref>], is a special transcendental function which has been found to occur in only a few experimental systems; thus,</p><disp-formula id="scirp.35103-formula150106"><label>(19)</label><graphic position="anchor" xlink:href="9-2710096\6c2bbe39-3637-4bc9-a148-9b0fddfe1d50.jpg"  xlink:type="simple"/></disp-formula><p>It can be evaluated through the following infinite series expansion for real positive arguments (x &gt; 0):</p><disp-formula id="scirp.35103-formula150107"><label>(20)</label><graphic position="anchor" xlink:href="9-2710096\bba1e3ef-60fb-436f-93a1-ba22e9a4c605.jpg"  xlink:type="simple"/></disp-formula><p>The Euler-Mascheroni constant (also called Euler’s constant) has been cited to be equal to 0.5772156649... It should be noted from Equation (20) that the Ei function approaches −∞ at its argument (x) approaching zero from the positive side (0<sup>+</sup>). This is reflected in inaccuracies in results from direct evaluation Equation (14) at τ → 0<sup>+</sup>.</p><p>In this paper, inaccuracies of the analytical evaluation of Equation (14) are addressed, by comparing predictions of the evolution of flat temperature profiles in FRRPP systems from numerical solutions and analytical approaches. Numerical solutions used include the evaluation of the field energy equation and its lumped-parameter version for a flat temperature profile. Analytical methods employed here include the use of the exponential integral function (Equation (14)), as well the TaylorSeries-based polynomial approximations.</p></sec><sec id="s2"><title>2. Generalized Mathematical Model of FRRPP Domains</title><p>Since the diffusive term could be neglected for the assumption of a flat temperature profile, then the geometry of the system does not matter and a lumped-parameter analysis can be made. In dimensional form the lumpedparameter energy balance around a reactive particle can be more conveniently expressed using the convective heat transfer coefficient, h, as</p><disp-formula id="scirp.35103-formula150108"><label>(21)</label><graphic position="anchor" xlink:href="9-2710096\273bfed2-10f2-4a47-85ba-9daf18d4dfbf.jpg"  xlink:type="simple"/></disp-formula><p>where A is the heat transfer area. For insulating boundary surfaces, h = 0, and thus</p><disp-formula id="scirp.35103-formula150109"><label>(22)</label><graphic position="anchor" xlink:href="9-2710096\7834f651-225b-4a77-9004-d908695f928b.jpg"  xlink:type="simple"/></disp-formula><p>Thus, the integral operation for the determination of τ at any value of Q is</p><disp-formula id="scirp.35103-formula150110"><label>(23)</label><graphic position="anchor" xlink:href="9-2710096\9fb3a0f6-7447-48a6-9cfa-abbb35e86bae.jpg"  xlink:type="simple"/></disp-formula><p>Equation (23) is used as the starting material for polynomial approximation at relatively small values of dimensionless time, τ, wherein the approximation is done with the integrand.</p></sec><sec id="s3"><title>3. Computer Simulation Results of IVP-PDE</title><p>In order to validate results of polynomial approximations of Equation (23), detailed field simulation results were also obtained. The following conditions have been deduced for the occurrence of a flat temperature profile in FRRPP systems:</p><p>1)<img src="9-2710096\f13d6825-6bde-4441-9471-2d50e22b5e8c.jpg" />, α &lt; 0, <img src="9-2710096\b51ba00b-4acf-4129-987b-d024e8faa213.jpg" />, <img src="9-2710096\b2c9791e-2347-4cac-8596-e6643b0b6de2.jpg" />, and h &gt; 0 2)<img src="9-2710096\580de769-b4a7-4809-8f65-c1e29ca7663e.jpg" />, α &lt; 0, <img src="9-2710096\b10a499f-28ed-473e-9671-7f9922a336d9.jpg" />, <img src="9-2710096\f98d805c-d04d-4c64-9f66-04b5c5514f99.jpg" />, and h = 0 3)<img src="9-2710096\d61ded49-e04f-45f9-b52e-a651b1a6a82d.jpg" />, α &gt; 0, <img src="9-2710096\70a44f0f-9fea-4bea-9de1-dc0432fb949b.jpg" />, <img src="9-2710096\bcb1e171-3fa3-484b-a0d2-d9f0652c40b1.jpg" />, and h = 0 Note that only Conditions 2 and 3 are covered in this paper.</p></sec><sec id="s4"><title>4. Polynomial Approximations from Early-Times Behavior</title><p>Let the function F(Q) correspond to the integrand of Equation (23); thus,</p><disp-formula id="scirp.35103-formula150111"><label>(24)</label><graphic position="anchor" xlink:href="9-2710096\fa64d75f-3940-4c0e-ad34-40527295cc6d.jpg"  xlink:type="simple"/></disp-formula><p>Application of the Taylor series expansion at the initial dimensionless time of zero and dimensionless temperature Q = 1 leads to</p><disp-formula id="scirp.35103-formula150112"><label>(25)</label><graphic position="anchor" xlink:href="9-2710096\77e10088-ac16-41e3-bba4-240984118b56.jpg"  xlink:type="simple"/></disp-formula><p>The software Mathematica<sup>&#174;</sup> is used to derive the various derivatives in Equation (25), and the following results were obtained up to the cubic derivative.</p><disp-formula id="scirp.35103-formula150113"><label>(26)</label><graphic position="anchor" xlink:href="9-2710096\ad1e6050-e750-47a7-8278-635e546a7c64.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150114"><label>(27)</label><graphic position="anchor" xlink:href="9-2710096\fd677842-ad08-471c-9074-3714f1bcf7f3.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35103-formula150115"><label>(28)</label><graphic position="anchor" xlink:href="9-2710096\0fcf53ec-9edd-43af-a42a-0dd66858c0bf.jpg"  xlink:type="simple"/></disp-formula><p>In order to understand the F(Q) function, it is plotted in <xref ref-type="fig" rid="fig3">Figure 3</xref> at typical parameter values for both stable and unstable systems, wherein the flat temperature profile is proposed to occur.</p><p>From this figure, the area under the curve can be obtained to be equal to the dimensionless time, t. Note that for the stable system, the value of Q approaches infinity at the steady-state value of 5. With the two sets of parameters in <xref ref-type="fig" rid="fig3">Figure 3</xref>, the resulting plots of the Dimensionless temperature, Q, vs Dimensionless time, t, is shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>.</p><p>Since the use of the Exponential Integral function, Ei, as defined in Equation (19), is not well understood in FRRPP systems, comparisons with straight numerical solution and Taylor Series approximations are made and reported in this paper. This exercise is very important for validation of a new conceptual phenomenon that is expressible with a rarely used transcendental function.</p></sec><sec id="s5"><title>5. Results of Polynomial Approximations</title><p>Figures 5(a) and 6(a) show polynomial approximation results of Q vs t for flat temperature profile histories involving typical stable and unstable parameter systems, which could be compared to numerical results in <xref ref-type="fig" rid="fig4">Figure 4</xref>. This stable system curve in <xref ref-type="fig" rid="fig4">Figure 4</xref>, in turn, has been found to compare very well with <xref ref-type="fig" rid="fig5">Figure 5</xref>(b), which is the numerical result of the solution of the full differential equation in Equation (22). For a representative unstable system, the dashed-curve result in <xref ref-type="fig" rid="fig4">Figure 4</xref> is compared with polynomial approximation results in <xref ref-type="fig" rid="fig6">Figure 6</xref>(a). This representative unstable system curve in <xref ref-type="fig" rid="fig4">Figure 4</xref>, in turn, has been found to compare well with <xref ref-type="fig" rid="fig6">Figure 6</xref>(b), which is the numerical result of the solution of the full differential equation in Equation (22). In addition, exponential integral results are shown for given parameter sets in Figures 5(a) and 6(a). Figures 7(a) and 7(b) show expanded abscissa scales for Figures 5(a) and 5(b), for additional comparisons. On the other hand, Figures 8(a) and 8(b) show shorter time behavior for conditions associated with Figures 6(a) and 6(b).</p><p>These plots indicate the validity of the use of the numerical approaches, compared to the Ei approximation method using Equation (14). If one uses the polynomial approximation, for a &lt; 0, the linear approximation would be quite accurate in the initial 60% - 70% Q-range, while the cubic approximation would be accurate in the initial 20% Q-range. For a &gt; 0, linear and cubic approximations seem to be accurate in the small-times range, or when Q &#174; 1. A point of caveat here is that the polynomial approximation does not seem to be asymptotic, until the cubic terms are reached. The final obvious point to be made here is that for a &lt; 0, the analytical-based Ei function is reasonably accurate at the above 20% Q-range.</p></sec><sec id="s6"><title>6. Conclusion</title><p>The quantitative analysis of the occurrence of the flat temperature profile in spherical FRRPP systems indicates that numerical approaches to predict its evolution would be reasonably accurate. If an analytical approximation is to be done, for a &lt; 0, the approach would be to use the linear Taylor series approximation up to 30% - 40% of the Q-range, and continuing to steady-state condition with the use of the Exponential Integral, Ei, function. For a &gt; 0, the only conclusion that can be made is that both linear and cubic polynomial approximations are reasonably accurate at very small times and low Q-values, i.e., at τ → 0 and Q &#174; 1.</p></sec><sec id="s7"><title>7. Acknowledgements</title><p>The authors are grateful for the support of the Michigan Tech Center for Environmentally Benign Functional Materials, the King Abdullah Scholarship Program, Najran and Michigan Tech Universities that allowed the continued work and publication of the quantitative investigation of the FRRPP process.</p></sec><sec id="s8"><title>REFERENCES</title></sec><sec id="s9"><title>1. Nomenclatures</title><sec id="s9_1"><title>1.1. Alphabets</title><sec id="s9_1_1"><title>1.1.1. Upper Case</title><p>A: Defined in Equation (8), dimensionless B: Defined in Equation (9), dimensionless E: Activation energy for reaction, J/mol F: Defined in Equation (24)</p><p>R: Universal gas constant, J/mol-K T: Absolute temperature, K X: Defined in Equations (10)-(11), dimensionless</p></sec><sec id="s9_1_2"><title>1.1.2. Lower Case</title><p>a: Defined in Equation (10)</p><p>b: Defined in Equation (10)</p><p>k: Thermal conductivity of the reaction fluid r: Radial distance, m or cm</p></sec></sec><sec id="s9_2"><title>1.2. Subscripts</title><p>a: pertains to Activation energy (Equation (5))</p><p>M: Pertains to monomer in Equation (11)</p><p>P: pertains to polymer in Equation (11)</p><p>0: pertains to Pre-exponential rate coefficient (Equations (3),(4),(8),(9)) or Dimensionless Energy Source Term ( Equation (12))</p></sec><sec id="s9_3"><title>1.3. Superscripts</title><p>P: Pertains to polymer-rich phase in Equation (11)</p></sec><sec id="s9_4"><title>1.4. Greek Symbols</title><p>α: Dimensionless version of a from Equation (3)</p><p>β: Dimensionless version of b from Equation (4)</p><p>γ: Dimensionless activation energy, defined in Equation (5)</p><p>η: Dimensionless radius, defined in Equation (7)</p><p>ρ: Density, g/cm<sup>3</sup> or kg/m<sup>3</sup></p><p>θ: Dimensionless temperature, defined in Equation (6)</p><p>Q: Dimensionless temperature, defined in Equation (16)</p><p>t: Dimensionless time, defined in Equation (15)</p><p>Φ: Dimensionless heat of polymerization, defined in Equation (2)</p></sec><sec id="s9_5"><title>1.5. Other Symbols</title><p><img src="9-2710096\07fdde7d-7016-496e-b6a3-f154890b8178.jpg" />: Defined in Equation (12), dimensionless Ei(x): Exponential integral function, defined in Equation (20)</p><p>f<sub>P</sub>: Polymer radical fraction</p><p>ΔH<sub>P</sub>: Heat of polymerization, J/mol k<sub>o</sub>’: Pre-exponential factor of rate coefficient, defined in Equations (3),(4),(8),(9)</p><p>k<sub>P</sub>: Propagation rate coefficient, Li/mol-s</p><p>Φ<sub>0</sub>: Dimensionless energy source term at the center of the particle, defined in Equation (12)</p><p>r<sub>0</sub>: Particle radius, cm or m X<sub>P</sub>: Defined in Equation (11)</p><p><img src="9-2710096\82f2ba28-c865-426f-89c1-3d04861b0ea2.jpg" />: Defined in Equation (11)</p><p><img src="9-2710096\c0c6b578-b7ac-4165-8b2d-c5a967051837.jpg" />: Defined in Equation (11)</p></sec></sec></body><back><ref-list><title>References</title><ref id="scirp.35103-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">G. 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