<?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">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2022.107153</article-id><article-id pub-id-type="publisher-id">JAMP-118723</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>
 
 
  Theoretical Study on the Effect of Multiband Structure on Critical Temperature and Electronic Specific Heat in SmOFeAs Iron Pnictide Superconductor
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shamin</surname><given-names>Masih</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>Piyush</surname><given-names>Masih</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sarita</surname><given-names>Khandka</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>SHUATS, Prayagraj, India</addr-line></aff><pub-date pub-type="epub"><day>11</day><month>07</month><year>2022</year></pub-date><volume>10</volume><issue>07</issue><fpage>2232</fpage><lpage>2244</lpage><history><date date-type="received"><day>24,</day>	<month>June</month>	<year>2022</year></date><date date-type="rev-recd"><day>23,</day>	<month>July</month>	<year>2022</year>	</date><date date-type="accepted"><day>26,</day>	<month>July</month>	<year>2022</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>
 
 
  In the present theoretical work, superconducting order parameter (
  &amp;#8710;) and electronic specific heat (
  <em>C<sub>es</sub></em>) of SmOFeAs iron pnictide (IP) superconductor has been studied using multiband (MB) model of IP superconductors. Attempt has been made to use the MB structure of IP superconductors and expressions for critical temperature (
  <em>T<sub>c</sub></em>) and 
  <em>C<sub>es</sub></em> are obtained, calculations being made for one, two and three bands of SmOFeAs. It has been found that MB results are close to the experimental value of 
  <em>T<sub>c</sub></em> for this compound. 
  <em>C<sub>es</sub></em> calculations show jump of 1.5 &#215; 10
  <sup>-5</sup> eV/atom K, 4 &#215; 10
  <sup>-5</sup> eV/atom K and 4 &#215; 10
  <sup>-5</sup> eV/atom K for one, two and three band models respectively. The study brings out the importance of MB structure in IPs, highlighting the fact that increasing the number of bands, increases 
  <em>T<sub>c</sub></em>. The specific heat jump (
  &amp;#8710;
  <em>C</em>) does not correspond to the BCS value, thereby proving that IPs are unconventional in nature.
 
</p></abstract><kwd-group><kwd>Electronic Specific Heat</kwd><kwd> Iron Pnictide Superconductor</kwd><kwd> Multiband</kwd><kwd> Superconducting Order Parameter</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The year 2006 [<xref ref-type="bibr" rid="scirp.118723-ref1">1</xref>] witnessed a major breakthrough in the field of superconductivity with the discovery of a new class of iron based superconductors called IPs. Further increase in T<sub>c</sub> in the same class of SCs was witnessed in the year 2008 [<xref ref-type="bibr" rid="scirp.118723-ref2">2</xref>]. Researchers all over the world were amused at the discovery made by Hideo Hosono [<xref ref-type="bibr" rid="scirp.118723-ref3">3</xref>] and coworkers in the course of exploration of magnetic semiconductors. These transition metal based superconductors having general formula LnOFeAs (Ln = La, Ce, Sm, Gd, Nd, Pr) are layered structures with alternate LnO &amp; FeAs layers, superconductivity believed to be present because of the FeAs layers. The structure orientation of Fe atoms shows it to be surrounded by four arsenic atoms resulting in a distorted tetrahedral geometry. The iron atoms are seen to make a square lattice and arsenic atoms are placed at the centre of each square being displaced above &amp; below the Fe planes. IPs are second in class after the cuprates [<xref ref-type="bibr" rid="scirp.118723-ref4">4</xref>] to have high T<sub>c</sub> of around 55 Kas shown by experimental studies of Ren and Chen [<xref ref-type="bibr" rid="scirp.118723-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref6">6</xref>] and theoretical study by Mebrahtu [<xref ref-type="bibr" rid="scirp.118723-ref7">7</xref>]. Interest in this newly class of discovered materials was generated not only because of its high T<sub>c</sub>, but also because iron, being the most magnetic material [<xref ref-type="bibr" rid="scirp.118723-ref8">8</xref>] that could have been destructive for superconductivity, showed high values of T<sub>c</sub>. Within a span of ten years, the quantum of research in this field is high because of the extraordinary properties exhibited by these compounds. It has been shown that in the normal state, these compounds are semi-metals [<xref ref-type="bibr" rid="scirp.118723-ref9">9</xref>] (upon doping [<xref ref-type="bibr" rid="scirp.118723-ref10">10</xref>] or application of pressure [<xref ref-type="bibr" rid="scirp.118723-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref14">14</xref>] is seen to increase T<sub>c</sub> in IPs). Several experimentation in this field is trying to study minutely various properties associated with them. Angle resolved photoemission experiments [<xref ref-type="bibr" rid="scirp.118723-ref15">15</xref>] have demonstrated that IPs are MB [<xref ref-type="bibr" rid="scirp.118723-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref17">17</xref>] in nature. Iron has five bands at the Fermi surface and all the five d-bands of iron are relevant in studying the superconducting properties of these compounds as opposed to the single band of cuprates [<xref ref-type="bibr" rid="scirp.118723-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref19">19</xref>] and BCS [<xref ref-type="bibr" rid="scirp.118723-ref20">20</xref>] superconductors or the two band MgB<sub>2</sub> [<xref ref-type="bibr" rid="scirp.118723-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref23">23</xref>]. Previous theories have found that MB nature [<xref ref-type="bibr" rid="scirp.118723-ref24">24</xref>] of IPs makes them a significant class in the vast area of superconductivity and that MB structure serves as an important ingredient for high T<sub>c</sub> [<xref ref-type="bibr" rid="scirp.118723-ref25">25</xref>] for this class of compounds. The four unpaired d electrons of iron are seen to hybridise [<xref ref-type="bibr" rid="scirp.118723-ref26">26</xref>] with the three unpaired p electrons of arsenic, resulting in bands found at the Fermi surface due to overlapping orbitals [<xref ref-type="bibr" rid="scirp.118723-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref28">28</xref>]. Raghu et al. has discussed that a minimal two band model [<xref ref-type="bibr" rid="scirp.118723-ref29">29</xref>] is needed for the superconducting IPs. Several others have also studied two bandsuperconductivity [<xref ref-type="bibr" rid="scirp.118723-ref30">30</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref32">32</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref33">33</xref>]. Three band superconductivities [<xref ref-type="bibr" rid="scirp.118723-ref34">34</xref>] have also been studied using different theories like Eliashberg theory [<xref ref-type="bibr" rid="scirp.118723-ref35">35</xref>], Ginzburg Landau theory [<xref ref-type="bibr" rid="scirp.118723-ref36">36</xref>], etc.</p><p>Over the years, the MB property of IPs is exploited in understanding these materials in a better way. Earlier, also it has been found that interband interactions lead to higher T<sub>c</sub> in cuprate SCs [<xref ref-type="bibr" rid="scirp.118723-ref37">37</xref>]. Since IPs are also MB SCs with nesting present at the Fermi surface, therefore it is desirable to investigate the role of interband and intraband interactions on various superconducting properties. Several properties of IPs are investigated to understand the mechanism of this special class of high temperature superconductors (HTS). The electronic specific heat of IPs is studied using electron-Cooper pair interaction by Mukubwa [<xref ref-type="bibr" rid="scirp.118723-ref38">38</xref>]. Mohamed et al. have explained pressure effect for HTS using pressure dependent Schrodinger equation and string theory [<xref ref-type="bibr" rid="scirp.118723-ref39">39</xref>]. With this motivation in mind, T<sub>c</sub> and C<sub>es</sub> of SmOFeAs compound [<xref ref-type="bibr" rid="scirp.118723-ref40">40</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref41">41</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref42">42</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref43">43</xref>] is investigated using a MB model, employing Green’s function technique and the results are compared with experimental values.</p></sec><sec id="s2"><title>2. Mathematical Technique and Formulation</title><p>In the present theoretical work, the two thermodynamical properties which is ∆ and C<sub>es</sub> of SmOFeAs are investigated as a function of the number of bands. The model Hamiltonian uses itinerant nature of electrons. It is described as:</p><p>H = ∑ m k σ E m k σ C m k σ + C m k σ − ∑ m k k ' V m m C m k ↑ + C m − k ↓ + C m − k ' ↓ C m k ' ↑     − V m n ∑ k k ' m ≠ n C m k ↑ + C m − k ↓ + C n − k ' ↓ C n k ' ↑ (1)</p><p>In Equation (1), the first term represents energy of itinerant electrons. The second term denotes the intraband interaction term. V<sub>mm</sub> is the intraband interaction potential. The third term is the interband interaction term. It represents tunnelling between the bands. V<sub>mn</sub> is the interband interaction potential. m, n is band index, k is wave vector and σ is spin index for fermions.</p><p>Considering the two Green’s functions</p><p>G r s ↑ q ↑ q = 〈 〈 C r q ↑ , C s q ↑ + 〉 〉 (2a)</p><p>G ↓ ↑ r s − q q = 〈 〈 C r − q ↓ + , C s q ↑ + 〉 〉 (2b)</p><p>Here r and s are the band index and q denotes wave vector.</p><p>Using the first Green function (2a), the equation of motion is expressed as:</p><p>( ω − E r q ↑ ) G r s ↑ q ↑ q = 1 2 π δ r s − V r r Δ r r G r ↓ s ↑ − q q − ∑ n r ≠ n V r n γ ↓ ↓ G n ↑ s q q ↑ − ∑ n r ≠ n V r n Δ n n G r ↓ s ↑ − q q (3)</p><p>Using the second Green function (2b), the second equation of motion is written as:</p><p>( ω + E r − q ↓ ) G r ↓ s ↑ − q q = − V r r Δ r r G r ↑ s ↑ q q − V r m ∑ m ≠ r m Δ m m G r ↑ s ↑ q q + V r m ∑ m ≠ r m γ ↑ ↑ G m ↓ s − ↑ q q (4)</p><p>where the OPs are defined as:</p><p>Δ r r = ∑ k ' 〈 C r − k ' ↓ , C r k ' ↑ 〉</p><p>Δ n n = ∑ k ' 〈 C n − k ' ↓ , C n k ' ↑ 〉</p><p>γ ↓ ↓ = ∑ k ' 〈 C r − q ↓ + , C n − k ' ↓ 〉</p><p>is number factor representing number of charge per unit volume.</p><sec id="s2_1"><title>2.1. One Band Model (OBM)</title><p>Using the two equations of Motion (3) and (4) and substituting r = s = 1 , calculations are done for OBM using E 1 q ↑ = E 1 − q ↓ and G 1 = G 11 q ↑ q ↑ and G 2 = G 11 − q ↓ q ↑</p><p>∆ is defined as:</p><p>Δ 11 = ∑ K V 11 〈 C 1 k ↑ + , C 1 − k ↓ + 〉 (5)</p><p>The correlation function (CF) 〈 C 1 k ↑ + , C 1 − k ↓ + 〉 is related to G<sub>2</sub> as:</p><p>〈 C 1 k ↑ + , C 1 − k ↓ + 〉 = − 1 i ∫ − ∞ ∞ G 2 ( ω + i ε ) − G 2 ( ω − i ε ) e ω k T − η (6)</p><p>where, η = − 1 for fermions, k is Boltzmann constant and T is absolute temperature in kelvin.</p><p>The expression of ∆ is obtained as:</p><p>Δ 11 = V 11 2 Δ 11 2 E 1 q ↑ 2 + ( V 11 Δ 11 ) 2 tanh E 1 q ↑ 2 + ( V 11 Δ 11 ) 2 2 k T (7)</p><p>Converting summation into integration with cut off energy &#177; ℏ ω D from the Fermi level and substituting T → T C as Δ → 0 :</p><p>1 = N 0 ∫ 0 ℏ ω D V 11 2 E 1 q ↑ tanh E 1 q ↑ 2 k T C d E 1 q ↑ (8)</p><p>T<sub>c</sub> can be expressed as:</p><p>1 = N O V 11 ∫ 0 ℏ ω D 1 2 E 1 q ↑ 2 + Δ &#175; 11 2 tanh E 1 q ↑ 2 + Δ &#175; 11 2 2 k T d E 1 q ↑ (9)</p><p>Here Δ &#175; 11 = V 11 Δ 11</p><p>For OBM, C<sub>es</sub> is defined as:</p><p>C e s 1 = ∂ ∂ T 1 N ∑ 2 E 1 q ↑ 〈 c 1 k ↑ + , c 1 k ↑ 〉 (10)</p><p>CF 〈 C 1 k ↑ + , C 1 k ↑ 〉 is related to G<sub>1</sub> as:</p><p>〈 C 1 k ↑ + , C 1 k ↑ 〉 = − 1 i ∫ − ∞ ∞ G 1 ( ω + i E ) − G 1 ( ω − i E ) e ω k T − η (11)</p><p>C<sub>es</sub> for OBM comes out as:</p><p>C e s 1 = 1 2 N k T 2 ∑ E 1 q ↑ 2 sech 2 ( E 1 q ↑ 2 + ( V 11 Δ 11 ) 2 2 k T ) (12)</p><p>Converting summation into integration,</p><p>C e s 1 = 1 N k T 2 ∫ 0 ℏ ω D E 1 q ↑ 2 sech 2 ( E 1 q ↑ 2 + ( V 11 Δ 11 ) 2 2 k T ) (13)</p></sec><sec id="s2_2"><title>2.2. Two Band Model (TBM)</title><p>Using the two equations of Motion (3) and (4) and substituting the four conditions: r = 1, s = 1; r = 1, s = 2; r = 2, s = 2 and r = 2, s =1, calculations are done for TBM using G 1 = G 11 q ↑ q ↑ , G 2 = G 11 − q ↓ q ↑ , G 3 = G 12 q ↑ q ↑ , G 4 = G 12 − q ↓ q ↑ , G 5 = G 22 q ↑ q ↑ , G 6 = G 22 − q ↓ q ↑ , E 1 q ↑ = E 1 − q ↓ and E 2 q ↑ = E 2 − q ↓</p><p>Similarly for TBM, the following results are obtained:</p><p>〈 C 1 k ↑ + , C 1 − k ↓ + 〉 = V 11 Δ 11 + V 12 Δ 22 2 E 1 q ↑ 2 + ( V 11 Δ 11 + V 12 Δ 22 ) 2 tanh E 1 q ↑ 2 + ( V 11 Δ 11 + V 12 Δ 22 ) 2 2 k T (14)</p><p>The second CF is obtained as:</p><p>〈 C 2 k ↑ + , C 2 − k ↓ + 〉 = V 21 Δ 11 + V 22 Δ 22 2 E 2 q ↑ 2 + ( V 21 Δ 11 + V 22 Δ 22 ) 2 tanh E 2 q ↑ 2 + ( V 21 Δ 11 + V 22 Δ 22 ) 2 2 k T (15)</p><p>C e s 21 comes out as:</p><p>C e s 21 = 1 2 N k T 2 Δ 1 Δ 2 ∑ E 1 q ↑ 2 sech 2 ( E 1 q ↑ 2 + Δ 1 2 2 k T ) (16)</p><p>Converting summation into integration,</p><p>C e s 21 = 1 N k T 2 Δ 1 Δ 2 ∫ 0 ℏ ω D E 1 q ↑ 2 sech 2 ( E 1 q ↑ 2 + Δ 1 2 2 k T ) (17)</p><p>C<sub>es</sub> for the second band corresponding to G<sub>5</sub> is defined as:</p><p>C e s 22 = ∂ ∂ T 1 N ∑ 2 E 2 q ↑ 〈 c 2 k ↑ + , c 2 k ↑ 〉 (18)</p><p>CF 〈 C 2 k ↑ + , C 2 k ↑ 〉 is related to G<sub>5</sub> as:</p><p>〈 C 2 k ↑ + , C 2 k 〉 = − 1 i ∫ − ∞ ∞ G 5 ( ω + i E ) − G 5 ( ω − i E ) e ω k T − η (19)</p><p>C e s 22 is calculated as:</p><p>C e s 22 = 1 2 N k T 2 ∑ E 2 q ↑ 2 sech 2 ( E 2 q ↑ 2 + Δ 2 2 2 k T ) (20)</p><p>Converting summation into integration,</p><p>C e s 22 = 1 N k T 2 ∫ 0 ℏ ω D E 2 q ↑ 2 sech 2 ( E 2 q ↑ 2 + Δ 2 2 2 k T ) (21)</p></sec><sec id="s2_3"><title>2.3. Three Band Model (THBM)</title><p>Using the two equations of Motion (3) and (4) and substituting the following eight conditions,<sub> </sub></p><p>r = 1, s = 1; r = 1, s = 2; r = 1, s = 3; r = 2, s = 1;r = 2, s = 2; r = 2, s = 3; r = 3,s = 1; r = 3, s = 2 and r = 3, s = 3, using the ten Green’s functions G<sub>1</sub> to G<sub>10</sub> and making following substitutions:</p><p>E 1 q ↑ = E 1 − q ↓ , E 21 q ↑ = E 2 − q ↓ , E 3 q ↑ = E 3 − q ↓</p><p>For the first band,</p><p>〈 C 1 k ↑ + , C 1 − k ↓ + 〉 = V 11 Δ 11 + V 12 Δ 22 + V 13 Δ 33 2 Δ 1 2 + ( E 1 q ↑ + V 12 V 31 V 32 γ ↑ ↑ ) 2 tanh Δ 1 2 + ( E 1 q ↑ + V 12 V 31 V 32 γ ↑ ↑ ) 2 2 k T (22)</p><p>For the second band, ∆ is obtained as:</p><p>Δ 22 = V 21 Δ 11 + V 22 Δ 22 + V 23 Δ 33 2 E 2 q ↑ 2 + ( V 21 Δ 11 + V 22 Δ 22 + V 23 Δ 33 ) 2     &#215; tanh E 2 q ↑ 2 + ( V 21 Δ 11 + V 22 Δ 22 + V 23 Δ 33 ) 2 2 k T (23)</p><p>For the third band, CF related to G<sub>10</sub> is written as:</p><p>〈 C 3 k ↑ + , C 3 − k ↓ + 〉 = − 1 i ∫ − ∞ ∞ G 10 ( ω + i ε ) − G 10 ( ω − i ε ) e ω K T − η (24)</p><p>The corresponding Δ 33 = V 33 〈 C 3 k ↑ + , C 3 − k ↓ + 〉 comes out to be:</p><p>Δ 33 = V 31 Δ 11 + V 32 Δ 22 + V 33 Δ 33 2 ( V 31 Δ 11 + V 32 Δ 22 + V 33 Δ 33 ) 2 + ( E 3 q ↑ + V 32 V 13 V 12 γ ↑ ↑ ) 2                 &#215; tanh ( V 31 Δ 11 + V 32 Δ 22 + V 33 Δ 33 ) 2 + ( E 1 q ↑ + V 32 V 13 V 12 γ ↑ ↑ ) 2 2 k T (25)</p><p>For THBM, expression for C e s 31 is:</p><p>C e s 31 = 1 2 N k T 2 ∑ E 1 q ↑ ( E 1 q ↑ + V 12 V 31 V 32 γ ) sech 2 ( ( E 1 q ↑ + V 12 V 31 V 32 γ ) 2 + Δ 1 2 2 K T ) (26)</p><p>Converting summation into integration gives:</p><p>C e s 31 = ∫ 0 ℏ ω D 1 N k T 2 E 1 q ↑ ( E 1 q ↑ + V 12 V 31 V 32 γ ) sech 2 ( ( E 1 q ↑ + V 12 V 31 V 32 γ ) 2 + Δ 1 2 2 K T ) (27)</p><p>C e s 32 is calculated as:</p><p>C e s 32 = 1 2 N k T 2 ∑ E 2 q ↑ 2 sech 2 ( E 2 q ↑ + Δ 2 2 2 k T ) (28)</p><p>Converting summation into integration,</p><p>C e s 32 = 1 N k T 2 ∫ 0 ℏ ω D E 2 q ↑ 2 sech 2 ( E 2 q ↑ + Δ 2 2 2 k T ) (29)</p><p>C<sub>es</sub> for the third band corresponding to G<sub>9</sub> is:</p><p>C e s 33 = ∂ ∂ T 1 N ∑ 2 E 3 q ↑ 〈 c 3 k ↑ + , c 3 k ↑ 〉 (30)</p><p>C e s 33 = 1 2 N k T 2 ∑ E 3 q ↑ ξ 2 − Δ 3 2 sech 2 ( E 3 q ↑ + V 32 V 13 V 12 γ ) 2 + Δ 3 2 2 k T (31)</p><p>Converting summation into integration,</p><p>C e s 33 = 1 N k T 2 ∫ 0 ℏ ω D E 3 q ↑ ( E 3 q ↑ + V 32 V 13 V 12 γ ) sech 2 ( E 3 q ↑ + V 32 V 13 V 12 γ ) 2 + Δ 3 2 2 k T (32)</p></sec></sec><sec id="s3"><title>3. Results and Discussion</title><p>In this section, the numerical results obtained for T<sub>c</sub> and C<sub>es</sub> of MB SmOFeAs are presented. The results are investigated as a function of the number of bands, expressions being obtained for one, two and three band models, highlighting the MB nature of the superconducting compound.</p><sec id="s3_1"><title>3.1. Variation of ∆ with T</title><p>∆ is a measure of the binding energy of Cooper pair. Its variation is studied with T as a function of the number of bands.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows the combined variation of ∆<sub>11</sub>, ∆<sub>22</sub> and ∆<sub>33</sub> with T for OB, TB and THBMs illustrating the rise in T<sub>c</sub> with increasing number of bands. It is seen that with increasing T, ∆ decreases and at T =T<sub>c</sub>, ∆ = 0<sub>.</sub> This is the usual behaviour of ∆ vs T and hence justified. T<sub>c</sub> for OBM comes out to be 11 K; for TBM, T<sub>c</sub> is 45 K and for THBM it is 57 K. During calculations, the values of ћω<sub>D</sub> = 0.05 eV, N = 10<sup>27</sup> eV/atom, N<sub>o</sub>V<sub>11</sub> = 0.24. N<sub>o</sub>V<sub>12</sub> = 0.12, N<sub>o</sub>V<sub>13</sub> = 0.06. The highest value of T<sub>c</sub> is seen to be 57 K which is very well in agreement with experimental results [<xref ref-type="bibr" rid="scirp.118723-ref5">5</xref>].</p></sec><sec id="s3_2"><title>3.2. Variation of C<sub>es</sub> with T</title><p>C<sub>es</sub> is the amount of heat per unit mass required to raise the temperature by one unit. Its variation is studied with T as a function of the number of bands.</p><p>Using Equation (13), the variation of C e s 1 with T for OBM shows that initially the SH for SC is less than the SH for normal state (NS), it then suddenly</p><p>increases and then drags down at a particular T which is the T<sub>c</sub> of the system which is 11 K as seen in the <xref ref-type="fig" rid="fig2">Figure 2</xref>. At T<sub>c</sub>, the curve shows a jump ∆C of 1.5 &#215; 10<sup>−5</sup> eV/atom K which is contrary as seen in the BCS model [<xref ref-type="bibr" rid="scirp.118723-ref44">44</xref>]. ∆C/ᵞT<sub>c</sub> is calculated as 1.101 for the model which is also not in accordance with BCS model [<xref ref-type="bibr" rid="scirp.118723-ref45">45</xref>], thus signifying that IPs are unconventional SCs [<xref ref-type="bibr" rid="scirp.118723-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref47">47</xref>].</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows the combined graph of the variation of C e s 21 and C e s 22 with T for TBM illustrating that initially the SH of SC is less than the SH for NS, it then suddenly increases at 7 K and then drags down atthe T<sub>c</sub> for the system, observed at 45 K. ∆C is 4 &#215; 10<sup>−5</sup> eV/atom K and ∆C/ᵞT<sub>c</sub> is calculated as 0.718 for the model. Both these values are not in accordance with BCS model, thereby showing that IPs are unconventional SCs.</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows the combined graph of the variation of C e s 31 , C e s 32 and C e s 33 with T for THBM illustrating that initially the SH of SC is less than the SH for NS, it then suddenly increases and then drags down at the T<sub>c</sub> for the system observed at 57 K. ∆C is 4 &#215; 10<sup>−5</sup> eV/atom K and ∆C/ᵞT<sub>c</sub> is calculated as 0.567 for the model. Both these values are not in accordance with BCS model proving IPs to be unconventional in nature. The value of Sommerfeld coefficientᵞ for the compound SmOFeAs is 119.4 mJ/mol K<sup>2</sup> [<xref ref-type="bibr" rid="scirp.118723-ref45">45</xref>].</p></sec></sec><sec id="s4"><title>4. Conclusion</title><p>The present study has been undertaken to get some information regarding the behaviour of T<sub>c</sub> and electronic specific heat for superconducting SmOFeAs. It is seen that upon increasing the number of bands has shown an increase in T<sub>c</sub> which is very well in agreement with experimental results, thereby proving that interband interactions play an important role in enhancing the T<sub>c</sub>. Thus this study also supports that MB structures are helpful to stabilize superconductivity and for obtaining high T<sub>c</sub> in this class of compounds. This appears reasonable as interband interactions are already found to enhance T<sub>c</sub> [<xref ref-type="bibr" rid="scirp.118723-ref25">25</xref>]. The specific heat calculations reveal that IPs are governed by a mechanism other than the BCS one [<xref ref-type="bibr" rid="scirp.118723-ref46">46</xref>]. The sharp peak observed in the specific heat curve is attributed to AFM ordering of Sm<sup>3+</sup> magnetic ions in the system which is otherwise not seen in the lanthanum compound that has non-magnetic La<sup>3+</sup> ions [<xref ref-type="bibr" rid="scirp.118723-ref47">47</xref>]. The theoretical model is restricted uptil three bands as suggested by Ummarino [<xref ref-type="bibr" rid="scirp.118723-ref35">35</xref>] that a simple THBM in strong-coupling regime [<xref ref-type="bibr" rid="scirp.118723-ref48">48</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref49">49</xref>] [<xref ref-type="bibr" rid="scirp.118723-ref50">50</xref>] can reproduce in a quantitative way the experimental T<sub>c</sub>.</p></sec><sec id="s5"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s6"><title>Cite this paper</title><p>Masih, S., Masih, P. and Khandka, S. 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