<?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">WJCMP</journal-id><journal-title-group><journal-title>World Journal of Condensed Matter Physics</journal-title></journal-title-group><issn pub-type="epub">2160-6919</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/wjcmp.2015.53017</article-id><article-id pub-id-type="publisher-id">WJCMP-58595</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>
 
 
  A Study of Superconducting La&lt;sub&gt;2&lt;/sub&gt;CuO&lt;sub&gt;4&lt;/sub&gt; via Generalized BCS Equations Incorporating Chemical Potential
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>.</surname><given-names>P. Malik</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>V.</surname><given-names>S. Varma</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Planning, Ambedkar University Delhi, Delhi, India</addr-line></aff><aff id="aff1"><addr-line>Theory Group, School of Environmental Sciences, Jawaharlal Nehru University, New Delhi, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>gulshanpmalik@yahoo.com, malik@jnu.ac.in(.PM)</email>;<email>varma2@gmail.com, vsvarma@aud.ac.in(VSV)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>27</day><month>07</month><year>2015</year></pub-date><volume>05</volume><issue>03</issue><fpage>148</fpage><lpage>159</lpage><history><date date-type="received"><day>16</day>	<month>June</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>2</month>	<year>August</year>	</date><date date-type="accepted"><day>5</day>	<month>August</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  We address the 
  <em>T</em>
  <sub><em>c</em></sub> (
  <em>s</em>) and multiple gaps of La
  <sub>2</sub>CuO
  <sub>4</sub> (LCO) via generalized BCS equations incorporating chemical potential. Appealing to the structure of the unit cell of LCO, which comprises sub- lattices with LaO and OLa layers and brings into play two Debye temperatures, the concept of itinerancy of electrons, and an insight provided by Tacon et al.’s recent experimental work concerned with YBa
  <sub>2</sub>Cu
  <sub>3</sub>O
  <sub>6.6</sub> which reveals that very large electron-phonon coupling can occur in a very narrow region of phonon wavelengths, we are enabled to account for all values of its gap-to-
  <em>T</em>
  <sub><em>c</em></sub> ratio (2Δ
  <sub>0</sub>/k
  <sub>B</sub>T
  <sub>c</sub>), i.e., 4.3, 7.1, ≈8 and 9.3, which were reported by Bednorz and M&#252;ller in their Nobel lecture. Our study predicts carrier concentrations corresponding to these gap values to lie in the range 1.3 &#215; 10
  <sup>21</sup> - 5.6 &#215; 10
  <sup>21</sup> cm
  <sup>-3</sup>, and values of 0.27 - 0.29 and 1.12 for the gap-to-
  <em>T</em>
  <sub><em>c</em></sub> ratios of the smaller gaps.
 
</p></abstract><kwd-group><kwd>Generalized BCS Equations</kwd><kwd> Chemical Potential</kwd><kwd> Two-Phonon Exchange Mechanism</kwd><kwd> Structure of the Unit Cell of LCO</kwd><kwd> Gap-to-&lt;i&gt;T&lt;sub&gt;c&lt;/sub&gt;&lt;/i&gt; Ratio</kwd><kwd> Effective Mass of Electrons</kwd><kwd> Number Densities of Charge Carriers</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>It is well known that La<sub>2</sub>CuO<sub>4</sub> (LCO) is an insulator. It becomes superconducting when suitably doped, (La<sub>0.925</sub>Sr<sub>0.075</sub>)<sub>2</sub>CuO<sub>4</sub> being an example which has a<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x6.png" xlink:type="simple"/></inline-formula>. Discovered by Bednorz and M&#252;ller [<xref ref-type="bibr" rid="scirp.58595-ref1">1</xref>] , it occupies a unique position among all the high-temperature superconductors (HTSCs) that have been discovered so far for the following reasons:</p><p>1) Being the first SC to transcend the BCS barrier of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x7.png" xlink:type="simple"/></inline-formula>, it heralded the era of high-T<sub>c</sub> superconductivity and led to the discovery of YBCO and the Tl-, Bi- and Hg-based SCs―each of them being characterized by a T<sub>c</sub> higher than even the liquefaction temperature of nitrogen. This of course is well known.</p><p>2) Unlike all the other HTSCs mentioned above, LCO contains predominantly only one species of ions that can give rise to pairing: La (strictly speaking, La<sub>0.925</sub>Sr<sub>0.075</sub>), which implies that pairing in it is governed by only one interaction parameter. This prima facie poses a problem because application of the generalized BCS equations [<xref ref-type="bibr" rid="scirp.58595-ref2">2</xref>] (GBCSEs) to an SC with a <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x8.png" xlink:type="simple"/></inline-formula> exceeding 23 K and possessing two gaps <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x9.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x10.png" xlink:type="simple"/></inline-formula> requires two-phonon exchange mechanism (TPEM) for pairing [<xref ref-type="bibr" rid="scirp.58595-ref3">3</xref>] ; by this we mean that phonons are exchanged with two distinct sub-lattice structures. For all the other HTSCs mentioned above, this brings into play two interaction parameters because their sub-lattices contain predominantly two distinct species of ions that can cause electron-phonon interaction to take place, e.g., Y and Ba ions [<xref ref-type="bibr" rid="scirp.58595-ref4">4</xref>] in YBa<sub>2</sub>CuO<sub>7</sub> and any two [<xref ref-type="bibr" rid="scirp.58595-ref3">3</xref>] of the Tl, Ba, and Ca ions in Tl<sub>2</sub>Ba<sub>2</sub>CaCuO<sub>8</sub>. This is also the case for the Bi-based [<xref ref-type="bibr" rid="scirp.58595-ref3">3</xref>] and iron-pnictide HTSCs [<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] .</p><p>3) When the problem mentioned above is addressed―by appealing to the structure of LCO as will be seen below―we find that the input of its T<sub>c</sub> alone yields an interaction parameter that enables one to calculate both its gaps. This is in contrast with all the other HTSCs for which the input of two parameters from the set <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x11.png" xlink:type="simple"/></inline-formula> is required to calculate the third.</p><p>The work reported here is motivated by the need to:</p><p>a) Bring the understanding of LCO in the framework of GBCSEs at par with that of all the other HTSCs noted above. This is done in the next section where for any T<sub>c</sub> in the range 37 - 40 K, it is shown, in accord with experiment, that 2∆<sub>20</sub>/k<sub>B</sub>T<sub>c</sub> = 4.3, where k<sub>B</sub> is the Boltzmann constant, and</p><p>b) Explain experimental values for the gap-to-T<sub>c</sub> ratio other than 4.3, i.e., 7.1, ≈8 and 9.3, attention to which was drawn by Bednorz and M&#252;ller [<xref ref-type="bibr" rid="scirp.58595-ref6">6</xref>] in their Nobel lecture. The study of these multiple gap-values is taken up in Section 3 by following an approach that incorporates the chemical potential μ into the equations for the ∆ and T<sub>c</sub> of the SC. Such an approach for LCO is based on 1) equations given in two recent papers, one [<xref ref-type="bibr" rid="scirp.58595-ref7">7</xref>] of which sheds light on the BCS-BES crossover physics without appeal to scattering length theory, while the other [<xref ref-type="bibr" rid="scirp.58595-ref8">8</xref>] suggests the possibility of solving a long-standing puzzle posed by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x12.png" xlink:type="simple"/></inline-formula> and 2) an idea inspired by another recent paper [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>] where it has been pointed out that a very large electron-phonon coupling occurs in a very narrow region of phonon wavelengths for an HTSC.</p><p>The final section is devoted to a discussion of our findings.</p></sec><sec id="s2"><title>2. LCO Addressed via GBCSEs</title><sec id="s2_1"><title>2.1. Debye Temperatures of La Ions in LCO</title><p>As noted [<xref ref-type="bibr" rid="scirp.58595-ref3">3</xref>] -[<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] for all the HTSCs dealt with so far, the first step in their study via GBCSEs is to fix the Debye temperatures of the ions that may be causing pairing. This is done by applying the following equations to each of the sub-lattices of the HTSC comprising layers designated as A<sub>x</sub>B<sub>1−x</sub>:</p><disp-formula id="scirp.58595-formula670"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x14.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula671"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x15.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x16.png" xlink:type="simple"/></inline-formula> is the Debye temperature of the HTSC, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x17.png" xlink:type="simple"/></inline-formula> is the atomic mass number of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x18.png" xlink:type="simple"/></inline-formula>. While Equation (1) has been used routinely for binary SCs, Equation (2) has been derived [<xref ref-type="bibr" rid="scirp.58595-ref2">2</xref>] by assuming that the constituents of any sub-lattice simulate the oscillations of a weakly coupled double pendulum. That the constituents of an anisotropic material must have different θ<sub>D</sub>s because their masses are different is an idea that dates back to Born and Karmann [<xref ref-type="bibr" rid="scirp.58595-ref10">10</xref>] .</p><p>The observation that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x19.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x20.png" xlink:type="simple"/></inline-formula> of an HTSC calculated via the above equations depend on the relative positions of A and B in the double pendulum suggests that the structure of the unit cell of the SC should be examined. On doing so we find that it is characterized by layers [<xref ref-type="bibr" rid="scirp.58595-ref11">11</xref>] of LaO, OLa, and CuO<sub>2</sub>. This implies that if La is the lower of the two bobs of the double pendulum in the layers that comprise one of the sub-lattices, it is the upper bob in the layers of the other sub-lattice. This feature brings into play two Debye temperatures, in the application of TPEM to LCO as for any of the other HTSCs, but only one interaction parameter because it is the same species of ions in both the sub-lattices that causes pairing.</p><p>Applying Equations (1) and (2) to the sub-lattice of LCO comprising OLa layers in which La is the lower of the two bobs, we find that [<xref ref-type="bibr" rid="scirp.58595-ref12">12</xref>] <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x21.png" xlink:type="simple"/></inline-formula>leads to</p><disp-formula id="scirp.58595-formula672"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x22.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x23.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x24.png" xlink:type="simple"/></inline-formula> have been used. The results for the sub-lattice comprising LaO layers are:</p><disp-formula id="scirp.58595-formula673"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x25.png"  xlink:type="simple"/></disp-formula></sec><sec id="s2_2"><title>2.2. Dealing with LCO with the Input of Its T<sub>c</sub></title><p>For the reason given above, GBCSE for T<sub>c</sub> of LCO in the two sub-lattice (two-phonon) scenario, obtained by putting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x26.png" xlink:type="simple"/></inline-formula> in Equation (4) of [<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] , is:</p><disp-formula id="scirp.58595-formula674"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x27.png"  xlink:type="simple"/></disp-formula><p>Note that the equivalent of Equation (5) for YBCO, for example, had two different interaction parameters: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula>. To determine these, the input of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula> and either <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x31.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x32.png" xlink:type="simple"/></inline-formula>―together with the corresponding θ<sub>D</sub>s―was required. One could then calculate the remaining parameter of the set<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x33.png" xlink:type="simple"/></inline-formula>. Since LCO is characterized by only one interaction parameter, it can be fixed via Equation (5) with the input of T<sub>c</sub> alone; we are then enabled to calculate both <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x34.png" xlink:type="simple"/></inline-formula><sub> </sub>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x29.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x35.png" xlink:type="simple"/></inline-formula>.</p><p>In writing Equation (5) we have dropped the superscripts of the two θs in the original equation. Solution of this equation with the input of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x36.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x37.png" xlink:type="simple"/></inline-formula>from Equation (3) and θ<sub>2</sub> = 431.1 K from Equation (4) yields</p><disp-formula id="scirp.58595-formula675"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x38.png"  xlink:type="simple"/></disp-formula><p>This leads to two values for the smaller gap and one for the larger gap via the following equations (Equations (3) and (5) of [<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] )</p><disp-formula id="scirp.58595-formula676"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x39.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula677"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x40.png"  xlink:type="simple"/></disp-formula><p>In these equations <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula> is to be identified with the smaller gap <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x42.png" xlink:type="simple"/></inline-formula><sub> </sub>at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x43.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x44.png" xlink:type="simple"/></inline-formula> with the larger gap <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x45.png" xlink:type="simple"/></inline-formula> at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x43.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x46.png" xlink:type="simple"/></inline-formula>; two values of the former are obtained because θ in Equation (7) can be either 104.8 or 431.1 K. Our results then are:</p><disp-formula id="scirp.58595-formula678"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x47.png"  xlink:type="simple"/></disp-formula><p>Because T<sub>c</sub> values of LCO reported in the literature vary from 36 - 40 K, we have given in <xref ref-type="table" rid="table1">Table 1</xref> not only the results of the above calculations for T<sub>c</sub> = 38 K, but also for four other values.</p></sec><sec id="s2_3"><title>2.3. Results with a Different Value of Debye Temperature</title><p>It was mentioned above that in giving an account of the properties of LCO, Bednorz and M&#252;ller in their Nobel lecture [<xref ref-type="bibr" rid="scirp.58595-ref6">6</xref>] had noted that besides 4.3 for the ratio<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x48.png" xlink:type="simple"/></inline-formula>, the following values have also been reported: 7.1, ≈ 8 and 9.3. While our result for this ratio is in agreement with the value 4.3 for any <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x49.png" xlink:type="simple"/></inline-formula> between 37 and 40 K, the problem of explaining the larger values remains. We note in this connection that the value of θ<sub>D</sub> (LCO)</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Values of the interaction parameter λ of superconducting La<sub>2</sub>CuO<sub>4</sub> obtained via Equation (5), and the associated gap-to-T<sub>c</sub> ratios for different values of T<sub>c</sub> obtained<sub> </sub>via Equations (8) and (7), respectively</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >T<sub>c</sub> (K)</th><th align="center" valign="middle" >λ</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x50.png" xlink:type="simple"/></inline-formula>(meV)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x51.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x52.png" xlink:type="simple"/></inline-formula>(meV)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x53.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x54.png" xlink:type="simple"/></inline-formula>(meV)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x55.png" xlink:type="simple"/></inline-formula></th></tr></thead><tr><td align="center" valign="middle" >36</td><td align="center" valign="middle" >0.26103</td><td align="center" valign="middle" >6.573</td><td align="center" valign="middle" >4.24</td><td align="center" valign="middle" >0.400</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" >1.647</td><td align="center" valign="middle" >1.06</td></tr><tr><td align="center" valign="middle" >37</td><td align="center" valign="middle" >0.26461</td><td align="center" valign="middle" >6.784</td><td align="center" valign="middle" >4.26</td><td align="center" valign="middle" >0.422</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" >1.737</td><td align="center" valign="middle" >1.09</td></tr><tr><td align="center" valign="middle" >38</td><td align="center" valign="middle" >0.26818</td><td align="center" valign="middle" >6.995</td><td align="center" valign="middle" >4.27</td><td align="center" valign="middle" >0.445</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >1.829</td><td align="center" valign="middle" >1.12</td></tr><tr><td align="center" valign="middle" >39</td><td align="center" valign="middle" >0.27173</td><td align="center" valign="middle" >7.207</td><td align="center" valign="middle" >4.29</td><td align="center" valign="middle" >0.467</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >1.922</td><td align="center" valign="middle" >1.14</td></tr><tr><td align="center" valign="middle" >40</td><td align="center" valign="middle" >0.27527</td><td align="center" valign="middle" >7.420</td><td align="center" valign="middle" >4.31</td><td align="center" valign="middle" >0.491</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >2.018</td><td align="center" valign="middle" >1.17</td></tr></tbody></table></table-wrap><p>employed in our study is 370 K, whereas values both smaller (360 K [<xref ref-type="bibr" rid="scirp.58595-ref12">12</xref>] ) and larger (385 K [<xref ref-type="bibr" rid="scirp.58595-ref13">13</xref>] ) have also been reported in the literature. It therefore seems pertinent to investigate the extent to which the gap-to-T<sub>c</sub> ratio changes if one were to adopt the largest of these values, i.e., 385 K. We have carried out this exercise with the following results:</p><disp-formula id="scirp.58595-formula679"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x56.png"  xlink:type="simple"/></disp-formula><p>From these results we conclude that all the different observed values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x57.png" xlink:type="simple"/></inline-formula> of LCO cannot be explained on the basis of variation in the Debye temperatures of its different samples.</p><p>This study of LCO in the framework of Equations (5) and (8) parallels earlier studies [<xref ref-type="bibr" rid="scirp.58595-ref3">3</xref>] -[<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] of various HTSCs in the same framework. Since at the end of it certain observed values of the gap-to-T<sub>c</sub> ratio remain unaccounted for, we are led to enlarge the framework employed by incorporating μ in the GBCSEs for ∆ and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x58.png" xlink:type="simple"/></inline-formula>. This is the task taken up in the next section.</p></sec></sec><sec id="s3"><title>3. LCO Addressed via μ-Incorporated GBCSEs</title><sec id="s3_1"><title>3.1. μ-Incorporated GBCSEs in the One-Phonon Exchange Mechanism (OPEM) Scenario for a 1-Component SC</title><p>It was remarked in [<xref ref-type="bibr" rid="scirp.58595-ref6">6</xref>] that the existence of CPs in LCO is an established experimental fact and that while more than one interaction for pairing may be operative, the phonon mechanism cannot be ruled out. Also reported in this paper is the value of the carrier density in one sample of LCO as being of the order of 10<sup>21</sup>/cm<sup>3</sup>, which is a parameter that is related to its Fermi energy. We now draw attention to the fact that Fermi energies of HTSCs have of late been attracting considerable interest, partly because their low values are believed [<xref ref-type="bibr" rid="scirp.58595-ref14">14</xref>] to be the cause of high-T<sub>c</sub>s and partly because they shed light on the gap-structures of HTSCs. In the context of LCO it seems significant that, on the basis of a thorough theoretical investigation, Jarlborg and Bianconi [<xref ref-type="bibr" rid="scirp.58595-ref15">15</xref>] have recently reported three values for its Fermi energy: 60, 150, and 240 meV. We now recall that both the usual BCS equations and GBCSEs, Equations (5) and (8) above, are derived by assuming</p><disp-formula id="scirp.58595-formula680"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x59.png"  xlink:type="simple"/></disp-formula><p>These considerations strongly suggest the need to study HTSCs in a more general framework of μ-incorpo- rated equations that are not constrained by the above inequality. Some of these equations are already available for studying pairing in the OPEM scenario; as was noted above, they were obtained in studies concerned with crossover physics and the superconductivity of SrTiO<sub>3</sub>. In this section we give a complete account of such equations in the OPEM scenario.</p><p>In the OPEM scenario, the μ-incorporated GBCSE at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x60.png" xlink:type="simple"/></inline-formula> for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x60.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x61.png" xlink:type="simple"/></inline-formula> (which is used interchangeably with ∆<sub>10</sub> in the equations below) is [<xref ref-type="bibr" rid="scirp.58595-ref7">7</xref>]</p><disp-formula id="scirp.58595-formula681"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x62.png"  xlink:type="simple"/></disp-formula><p>where V<sub>0</sub> is the BCS interaction parameter as in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x63.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x64.png" xlink:type="simple"/></inline-formula> the chemical potential at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x63.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x65.png" xlink:type="simple"/></inline-formula>, and</p><disp-formula id="scirp.58595-formula682"><graphic  xlink:href="http://html.scirp.org/file/5-4800309x66.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula683"><graphic  xlink:href="http://html.scirp.org/file/5-4800309x67.png"  xlink:type="simple"/></disp-formula><p>Substituting these into Equation (12) and multiplying with<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x68.png" xlink:type="simple"/></inline-formula>, we have</p><disp-formula id="scirp.58595-formula684"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x69.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.58595-formula685"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x70.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.58595-formula686"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x71.png"  xlink:type="simple"/></disp-formula><p>From the following relations involving the number density of conduction electrons and other relevant parameters</p><disp-formula id="scirp.58595-formula687"><graphic  xlink:href="http://html.scirp.org/file/5-4800309x72.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula688"><graphic  xlink:href="http://html.scirp.org/file/5-4800309x73.png"  xlink:type="simple"/></disp-formula><p>we obtain</p><disp-formula id="scirp.58595-formula689"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x74.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.58595-formula690"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x75.png"  xlink:type="simple"/></disp-formula><p>The last step is a consequence of splitting the region of integration into two parts (when<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula>): <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x77.png" xlink:type="simple"/></inline-formula>to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x78.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x79.png" xlink:type="simple"/></inline-formula> to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x80.png" xlink:type="simple"/></inline-formula>; in the first part <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x77.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x79.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x80.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x81.png" xlink:type="simple"/></inline-formula> whence the expression in the square brackets in the integrand reduces to 2.</p><p>From Equations (13) and (16) we obtain</p><disp-formula id="scirp.58595-formula691"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x82.png"  xlink:type="simple"/></disp-formula><p>Equation (18), valid at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x83.png" xlink:type="simple"/></inline-formula>, is one of our basic equations. Given below from [<xref ref-type="bibr" rid="scirp.58595-ref8">8</xref>] is another basic equation which is valid at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x84.png" xlink:type="simple"/></inline-formula>:</p><disp-formula id="scirp.58595-formula692"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x85.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.58595-formula693"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x86.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula694"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x87.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.58595-formula695"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x88.png"  xlink:type="simple"/></disp-formula><p>In the above equations μ<sub>1</sub> is the chemical potential and V<sub>1</sub> the value of V in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x89.png" xlink:type="simple"/></inline-formula> at<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x89.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x90.png" xlink:type="simple"/></inline-formula>.</p><p>If μ<sub>1</sub> and T<sub>c</sub> are known, then we can determine <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x91.png" xlink:type="simple"/></inline-formula> via</p><disp-formula id="scirp.58595-formula696"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x92.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3_2"><title>3.2. μ-Incorporated GBCSEs in the Two-Phonon Exchange Mechanism (TPEM) Scenario for a Composite SC</title><p>Equations (18) and (19) can be generalized to the TPEM scenario by replacing the “propagator” V used in the former scenario by a “superpropagator” <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula>[<xref ref-type="bibr" rid="scirp.58595-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.58595-ref16">16</xref>] , where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula> for electrons in the energy range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x95.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x96.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x97.png" xlink:type="simple"/></inline-formula> in the range <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x98.png" xlink:type="simple"/></inline-formula> to<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x94.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x98.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x99.png" xlink:type="simple"/></inline-formula>; otherwise these interaction parameters have vanishing values. Following then the procedure given in [<xref ref-type="bibr" rid="scirp.58595-ref16">16</xref>] , we obtain for LCO (which we recall involves only one interaction parameter) the following equation as generalization of Equation (18)</p><disp-formula id="scirp.58595-formula697"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x100.png"  xlink:type="simple"/></disp-formula><p>where the superscript (2) of a symbol denotes that it pertains to the TPEM scenario, and</p><disp-formula id="scirp.58595-formula698"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x101.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58595-formula699"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x102.png"  xlink:type="simple"/></disp-formula><p>In these equations θ<sub>1</sub> and θ<sub>2</sub> are the values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x103.png" xlink:type="simple"/></inline-formula> given in Equations (3) and (4), respectively, and the upper limit of the number equation has been taken as the greater of the two Debye temperatures so that pairing can take place due to both the sub-lattices.</p><p>Similarly, we obtain the desired generalization of Equation (19) as</p><disp-formula id="scirp.58595-formula700"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x104.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.58595-formula701"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x105.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.58595-formula702"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x106.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3_3"><title>3.3. An explanation of the Result <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x107.png" xlink:type="simple"/></inline-formula> = 4.27 for LCO on the Basis of Equations (24) and (27) and a Tenet of BCS Theory</title><p>While our treatment of the pairing problem in both OPEM and TPEM scenarios has been perfectly general, it has led to an undetermined set of equations. In the latter case we have only two equations, Equations (24) and (27), containing six variables: λ<sub>0</sub>, λ<sub>1</sub>, μ<sub>0</sub>, μ<sub>1</sub>, W<sub>20</sub>, and T<sub>c</sub>. Therefore we now assume</p><disp-formula id="scirp.58595-formula703"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x108.png"  xlink:type="simple"/></disp-formula><p>We could have made this assumption at the outset because it is in accord with a tenet of BCS theory. We chose not to do so in order to have readily available a set of equations that might be useful, should it be considered worthwhile to follow up this work with one of greater generality. All calculations in the following are carried out by assuming Equation (30).</p><p>Since Equations (24) and (27) are the μ-incorporated versions of Equations (8) and (5), respectively, we need to show that when the constraint embodied in Equation (11) is imposed they yield solutions in agreement with those obtained by solving the latter equations. To this end, we solve Equation (27) for λ with the input of θ<sub>1</sub> = 104.8 K, θ<sub>2</sub> = 431.1 K (see Equations (3) and (4)), T<sub>c</sub> = 38 K and different values of μ. We begin with μ = 300 k<sub>B</sub>θ<sub>2</sub>, which manifestly satisfies Equation (11), and find that λ = 0.26818, which is the result that we had obtained earlier via Equation (5) and noted in Equation (6). Solution of Equation (24) with μ = 300 k<sub>B</sub>θ<sub>2</sub>, and λ = 0.26818 then yields <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x109.png" xlink:type="simple"/></inline-formula> = 6.995 meV, or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x110.png" xlink:type="simple"/></inline-formula>, which also agrees with the result obtained earlier via Equation (8) and noted in Equation (9). Having thus established that Equations (24) and (27) satisfy the requisite consistency condition, repeating the exercise just carried out by progressively decreasing μ we find that (a) all results quoted for μ = 300 k<sub>B</sub>θ<sub>2</sub> remain unchanged for values of μ up to ≈ 40 meV, and (b) for the limiting value of μ = k<sub>B</sub>θ<sub>2</sub> = 37.15 meV (note that any value lower than this will cause <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x111.png" xlink:type="simple"/></inline-formula> to become complex − see Equation (28)), the results are: λ = 0. 27507, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x112.png" xlink:type="simple"/></inline-formula>= 6.953 meV, or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x109.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x111.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x113.png" xlink:type="simple"/></inline-formula>.</p><p>Even after incorporating μ in the equations for T<sub>c</sub> and ∆, our considerations so far have succeeded in explaining only one of the observed values of the gap-to-T<sub>c</sub> ratio for LCO. Therefore there would seem to be a need for a new idea to explain the other values. It seems to us that the recent findings of Tacon et al. [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>] provide precisely such an idea, even though they are based on experiments carried out with another HTSC (YBa<sub>2</sub>Cu<sub>3</sub>O<sub>6.6</sub>). Appealing to it while solving Equations (24) and (27), we present in the next section a complete solution of the problem being addressed.</p></sec><sec id="s3_4"><title>3.4. An Explanation of the Different Reported Values of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x114.png" xlink:type="simple"/></inline-formula> for LCO Based on a Treatment of the Number Equations at T = T<sub>c</sub> and T = 0 in the Light of the Experimental Findings of Tacon et al. [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>]</title><p>The work reported in this section is based on an idea inspired by Tacon et al.’s experimental findings about the role of low-energy phonons in YBa<sub>2</sub>Cu<sub>3</sub>O<sub>6.6</sub> (superconducting transition temperature T<sub>c</sub> =  61 K) determined by employing high-resolution inelastic X-ray scattering. These experiments revealed features that were interpreted by the authors as signifying that (a) extremely large superconductivity-induced line-shape renormalizations are caused by phonons in a narrow range of momentum space and (b) the electron-phonon interaction has sufficient strength to generate various anomalies in electronic spectra, but does not contribute significantly to Cooper pairing. Having probed the electron-phonon coupling via their ingenious two-level approach of X-ray scattering, they further noted that “in terms of its amplitude, the coupling is actually by far the biggest ever observed in a superconductor, but it occurs in a very narrow region of phonon wavelengths and at a very low energy of vibration of the atoms”. This statement induces us to review below our earlier treatment of the number equation.</p><p>We recall that the limits of the number equation in the previous section―both at T = T<sub>c</sub> and T = 0―were taken as −μ and k<sub>B</sub>θ<sub>2</sub>. We now call attention to the facts that a) in dealing with an SC that has T<sub>c</sub> ≈ 38 K, we need to invoke TPEM, which b) brings into play two Debye temperatures θ<sub>1</sub> and θ<sub>2</sub> &gt; θ<sub>1</sub>, and c) if the SC were a 1-component SC characterized by θ<sub>1</sub>, the number equation at T = 0 for it would comprise two terms: one corresponding to where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x115.png" xlink:type="simple"/></inline-formula> = 0 for electrons having energies between −μ and −k<sub>B</sub>θ<sub>1 </sub>and the other where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x116.png" xlink:type="simple"/></inline-formula> ≠ 0 for energies between −k<sub>B</sub>θ<sub>1</sub> and +k<sub>B</sub>θ<sub>1</sub> (see Equation (17)); similarly, if the SC was a 1-component SC characterized by θ<sub>2</sub>, the number equation for it at T = 0 would comprise two terms, one corresponding to where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x117.png" xlink:type="simple"/></inline-formula> = 0 for energies between −μ and −k<sub>B</sub>θ<sub>2</sub> and the other where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x118.png" xlink:type="simple"/></inline-formula> ≠ 0 for energies between −k<sub>B</sub>θ<sub>2</sub> and +k<sub>B</sub>θ<sub>2</sub>. Note that the lower limit in both these cases is −μ. In dealing with a composite SC characterized by two Debye temperatures θ<sub>1</sub> and θ<sub>2</sub> &gt; θ<sub>1</sub>, it was then natural to take k<sub>B</sub>θ<sub>2</sub> as the upper limit of the number equation, and this is the choice we had made earlier.</p><p>Guided by the insight provided by the findings of Tacon et al. [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>] , we now proceed to explore the consequences of narrowing down the range of phonon energies in the problem. If we require that in doing so we should keep intact for both the sub-lattices the region of momentum space for which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x119.png" xlink:type="simple"/></inline-formula> ≠ 0, then we need to make just one change in our earlier treatment of the number equations: drop the first term in Equation (26). We recall that this term corresponds to the region for which <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x120.png" xlink:type="simple"/></inline-formula> = 0. We now follow up on this idea.</p><p>Our procedure above comprised solving Equation (27) for λ with the input of T<sub>c</sub> and different values of μ and then using these (λ, μ) values to solve Equation (24) for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x121.png" xlink:type="simple"/></inline-formula>. We now adopt a variant of this procedure which comprises (a) eliminating λ from Equations (24) and (27) by appealing to Equation (30), (b) solving the resulting equation for μ with the input of T<sub>c</sub> = 38 K and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x121.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x122.png" xlink:type="simple"/></inline-formula> with p as a variable, and then (c) determining λ by using either Equation (24) or (27). This is a procedure that enables us to find quickly if sensible solutions for (λ, μ) exist for any particular value of p.</p><p>Eliminating λ from Equations (24) and (27) by appealing to Equation (30), we have</p><disp-formula id="scirp.58595-formula704"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x123.png"  xlink:type="simple"/></disp-formula><p>Attempting to solve Equation (31), we find that it has no solution for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x124.png" xlink:type="simple"/></inline-formula>. The solutions for μ for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x125.png" xlink:type="simple"/></inline-formula> have been shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>. The μ values of this figure are used to calculate the coupling strength λ [with the additional input of θ<sub>1</sub> = 104.8 K, θ<sub>2</sub> = 431.1 K, and T<sub>c</sub> = 38 K)] via Equation (24) whence it is found to lie in the range 0.27388 - 0.26843. The resulting plot of λ against p is shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>. In <xref ref-type="table" rid="table2">Table 2</xref>, we have given the (μ, λ) solutions corresponding to the four specific values of p, i.e., 4.3, 7.1, 8, and 9.3, that were mentioned in [<xref ref-type="bibr" rid="scirp.58595-ref6">6</xref>] . These results change insignificantly if T<sub>c</sub> is taken as 36 K or 40 K (rather than 38 K) as is seen from the following examples:</p><disp-formula id="scirp.58595-formula705"><graphic  xlink:href="http://html.scirp.org/file/5-4800309x126.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s4"><title>4. Predictions of the μ-Incorporated GBCSEs for LCO</title><sec id="s4_1"><title>4.1. Values of the Smaller Gaps</title><p>A review of our procedure so far is as follows. By including μ in GBCSEs as applicable to LCO, appealing to an idea inspired by the work of Tacon et al. [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>] and using as input any of the observed values of the gap-to-T<sub>c</sub> ratio for 36 ≤ T<sub>c</sub> ≤ 40 K, we have been led to solutions for μ and λ that are “sensible”. Sensible because we found a) μ to have a low value―in the meV range (recall that for elemental SCs, μ is in ≈2 - 10 eV range), which is in accord with the assertion made in [<xref ref-type="bibr" rid="scirp.58595-ref14">14</xref>] and the values reported in [<xref ref-type="bibr" rid="scirp.58595-ref15">15</xref>] , and b) λ to be less than 0.5, which is in accord with the Bogoliubov constraint as discussed in [<xref ref-type="bibr" rid="scirp.58595-ref5">5</xref>] .</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Plot of the chemical potential μ (meV) for different values of p obtained by solving Equation (30) with the input of θ<sub>1</sub> = 104.8 K, θ<sub>2</sub> = 431.1 K, T<sub>c</sub> = 38 K, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x128.png" xlink:type="simple"/></inline-formula></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-4800309x127.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Plot of the coupling strength λ against p obtained by solving Equation (24) with the input of μ values from the (μ, p) plot of <xref ref-type="fig" rid="fig1">Figure 1</xref>, θ<sub>1</sub> = 104.8 K, θ<sub>2</sub> = 431.1 K, and T<sub>c</sub> = 38 K</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/5-4800309x129.png"/></fig><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Values of μ obtained by solving Equation (31) in the TPEM scenario with the input of θ<sub>1</sub> = 104.8 K, θ<sub>2</sub> = 431.1 K, T<sub>c</sub> = 38 K, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x130.png" xlink:type="simple"/></inline-formula>(p = 4.3, 7.1, etc.) and the corresponding values of λ calculated via Equation (24) or (27). Each pair of these (μ, λ) values is then used to calculate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x131.png" xlink:type="simple"/></inline-formula> in the OPEM scenario by using Equation (18), first by taking θ as 104.8 K and then 431.1 K. Adjacent to each value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x131.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x132.png" xlink:type="simple"/></inline-formula> is given in parentheses the temperature at which it is calculated via Equation (19) to vanish. In the columns following these values are given the corresponding gap-to-T<sub>c</sub> ratios with T<sub>c</sub> taken as 38 K, i.e., the temperature at which the larger gap vanishes</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x133.png" xlink:type="simple"/></inline-formula></th><th align="center" valign="middle"  colspan="2"  >TPEM scenario</th><th align="center" valign="middle"  colspan="4"  >OPEM scenario</th></tr></thead><tr><td align="center" valign="middle" ></td><td align="center" valign="middle"  colspan="2"  ></td><td align="center" valign="middle"  colspan="2"  ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x134.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle"  colspan="2"  ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x135.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x136.png" xlink:type="simple"/></inline-formula>(meV)</td><td align="center" valign="middle" >λ</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x137.png" xlink:type="simple"/></inline-formula>, meV (T<sub>c</sub>, K)</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x138.png" xlink:type="simple"/></inline-formula></td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x139.png" xlink:type="simple"/></inline-formula>, meV (T<sub>c</sub>, K)</td><td align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x140.png" xlink:type="simple"/></inline-formula></td></tr><tr><td align="center" valign="middle" >4.3</td><td align="center" valign="middle" >39.72</td><td align="center" valign="middle" >0.27388</td><td align="center" valign="middle" >0.480 (3.1)</td><td align="center" valign="middle" >0.293</td><td align="center" valign="middle" >1.85 (11.9)</td><td align="center" valign="middle" >1.13</td></tr><tr><td align="center" valign="middle" >7.1</td><td align="center" valign="middle" >104.4</td><td align="center" valign="middle" >0.26886</td><td align="center" valign="middle" >0.449 (2.9)</td><td align="center" valign="middle" >0.274</td><td align="center" valign="middle" >1.83 (11.8)</td><td align="center" valign="middle" >1.12</td></tr><tr><td align="center" valign="middle" >8.0</td><td align="center" valign="middle" >127.8</td><td align="center" valign="middle" >0.26862</td><td align="center" valign="middle" >0.447 (2.9)</td><td align="center" valign="middle" >0.273</td><td align="center" valign="middle" >1.83 (11.8)</td><td align="center" valign="middle" >1.12</td></tr><tr><td align="center" valign="middle" >9.3</td><td align="center" valign="middle" >165.2</td><td align="center" valign="middle" >0.26846</td><td align="center" valign="middle" >0.446 (2.9)</td><td align="center" valign="middle" >0.273</td><td align="center" valign="middle" >1.83 (11.8)</td><td align="center" valign="middle" >1.12</td></tr></tbody></table></table-wrap><p>We now note that the (μ, λ)-values that we have been led to, enable us to calculate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x141.png" xlink:type="simple"/></inline-formula> and T<sub>c</sub> in the OPEM scenario vide Equations (18) and (19), respectively. These results, which constitute predictions of our approach, are also included in <xref ref-type="table" rid="table2">Table 2</xref>. It thus follows that, in suitably sensitized experimental set-ups, LCO should also exhibit for the gap-to-T<sub>c</sub> ratio (with T<sub>c</sub> taken as 38 K) the following values: 0.27 - 0.29 (≈3 K) and 1.12 (≈12 K), where the numbers in the parentheses denote the temperatures at which these smaller gaps are predicted to vanish.</p></sec><sec id="s4_2"><title>4.2. Carrier Concentration</title><p>We can calculate the carrier concentration n via the following equation</p><disp-formula id="scirp.58595-formula706"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x142.png"  xlink:type="simple"/></disp-formula><p>which is the second equation after Equation (15), with E<sub>F</sub> replaced by μ and the factor of ħ<sup>2</sup> inserted. However, before we can use this equation we need to find the band effective mass of electrons in LCO. This can be done by using the following expressions for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x143.png" xlink:type="simple"/></inline-formula> as in <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x143.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x144.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.58595-formula707"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x145.png"  xlink:type="simple"/></disp-formula><p>where we have put the band effective mass as s times the free electron mass m<sub>e</sub>, and</p><disp-formula id="scirp.58595-formula708"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x146.png"  xlink:type="simple"/></disp-formula><p>where γ is the experimentally obtained electronic specific heat constant (also known as the Sommerfeld constant) and v the gm-at volume.</p><p>From Equations (33) and (34) we obtain</p><disp-formula id="scirp.58595-formula709"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x147.png"  xlink:type="simple"/></disp-formula><p>We now use: γ = 4.5 mJ/mol K<sup>2</sup> (given in [<xref ref-type="bibr" rid="scirp.58595-ref11">11</xref>] ), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/5-4800309x148.png" xlink:type="simple"/></inline-formula>= 22.60 cm<sup>3</sup> and the values of μ corresponding to p = 4.3 and 9.3 to obtain</p><disp-formula id="scirp.58595-formula710"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x149.png"  xlink:type="simple"/></disp-formula><p>Upon putting m = s times the free electron mass in Equation (32) we obtain</p><disp-formula id="scirp.58595-formula711"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/5-4800309x150.png"  xlink:type="simple"/></disp-formula><p>Since the value of the carrier concentration noted in [<xref ref-type="bibr" rid="scirp.58595-ref6">6</xref>] is “of the order of 10<sup>21</sup>/cm<sup>3</sup>,” these results support the approach followed in this study.</p></sec></sec><sec id="s5"><title>5. Discussion</title><p>1) Strictly speaking, Fermi energy is a term applicable to non-interacting systems. In this note however it has been used interchangeably with the chemical potential, as is usually done in the literature on superconductivity.</p><p>2) It is well known that HTSCs are characterized by multiphase and multi-scale complexity and that their Fermi surfaces have highly complex structures comprising many sheets that span different bands. In the light of this observation it would seem that our treatment of LCO based on multiple Debye temperatures and TPEM is rather naive. We are therefore impelled to draw attention to the following:</p><p>a) As can be seen in [<xref ref-type="bibr" rid="scirp.58595-ref17">17</xref>] , Fermi surfaces of elemental SCs too have rather complex structures: none of them has the idealized spherical Fermi surface assumed in BCS theory. And yet, with the exception of a few, e.g., Pb and Hg, the mean-field approximation (MFA) employed in the theory works for most of them.</p><p>b) It is evident that the values of μ corresponding to different values of ∆<sub>2</sub> and T<sub>c</sub> that we have determined reflect the structure of the Fermi surface of the SC. Implicit in our approach is the concept of locally spherical Fermi surfaces (LSFSs), which takes the complexity of the HTSC into account in a rather simple (if not the simplest possible) manner. Such simplicity of approach for the kind of system we are dealing with is a goal every model strives to achieve. We note that LSFSs come into play because of itinerancy of electrons and the adoption of MFA.</p><p>c) Itinerancy of electrons in a multi-band SC is a much-invoked concept since at least the time of Suhl et al.’s paper [<xref ref-type="bibr" rid="scirp.58595-ref18">18</xref>] . We give below an analogy to bring out how this concept justifies dropping of the first term in the number equation (26).</p><p>d) Consider a convoy on a road passing through a range of mountains. As the road twists and turns through a series of valleys and mountains, the amount of sunlight it receives will vary from a maximum at the highest point of the range to a minimum at a place determined by the topography of the entire range. Itinerant conduction electrons in a solid on a 3-D Fermi surface are akin to such a convoy: there will be places where they can exchange phonons with the A- or the B-ions separately, and a place or places where they can exchange phonons with both of them simultaneously. For the last of these cases, one can then envisage a situation where phonon energies span not the usual range from −μ to k<sub>B</sub>θ<sub>2</sub>, but a depleted range from −k<sub>B</sub>θ<sub>2</sub> to k<sub>B</sub>θ<sub>2</sub>. The mean value of μ for the electrons under consideration is equivalent to the word “place” used for the convoy.</p><p>e) It seems interesting to point out that the concept of LSFSs is similar to the concept of locally inertial coordinate frames employed in the general theory of relativity [<xref ref-type="bibr" rid="scirp.58595-ref19">19</xref>] .</p><p>3) In connection with the remark by Tacon et al. [<xref ref-type="bibr" rid="scirp.58595-ref9">9</xref>] that “the electron-phonon interaction has sufficient strength to generate various anomalies in electronic spectra, but does not contribute significantly to Cooper pairing”, we should like to note that this statement is presumably based keeping OPEM in mind, which cannot account for the observed T<sub>c</sub> of LCO.</p></sec><sec id="s6"><title>6. Conclusions</title><p>Our findings provide a confirmation of the idea that low values of μ play an important role in HTSCs. Besides, we have for the first time given a plausible quantitative explanation of the different values of gap-to-T<sub>c</sub> ratio that have been reported for LCO in the literature.</p><p>In effect, the approach followed in this note can also be viewed as a new direct method for relating the ∆<sub>0</sub> and T<sub>c</sub> of an HTSC with its E<sub>F</sub>.</p></sec><sec id="s7"><title>Acknowledgements</title><p>G. P. M. acknowledges that his correspondence with Dr. D. M. Eagles and Professor M. de Llano has been invaluable in this study. He thanks Professor G. Szirmai for a perceptive remark during EUROQUAM 2010 on the approach followed herein and Professor D. C. Mattis for encouragement.</p></sec><sec id="s8"><title>Cite this paper</title><p>G. P.Malik,V. S.Varma, (2015) A Study of Superconducting La<sub>2</sub>CuO<sub>4</sub> via Generalized BCS Equations Incorporating Chemical Potential. World Journal of Condensed Matter Physics,05,148-159. doi: 10.4236/wjcmp.2015.53017</p></sec><sec id="s9"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.58595-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Bednorz, J.G. and Müller, K.A. (1986) Possible High Tc Superconductivity in Ba-La-Cu-O System. Zeitschrift für Physik B Condensed Matter, 64, 189-193. http://dx.doi.org/10.1007/BF01303701</mixed-citation></ref><ref id="scirp.58595-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. (2010) On the Equivalence of the Binding Energy of a Cooper Pair and the BCS Energy Gap: A Framework for Dealing with Composite Superconductors. International Journal of Modern Physics B, 24, 1159-1172. 
http://dx.doi.org/10.1142/S0217979210055408</mixed-citation></ref><ref id="scirp.58595-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. and Malik, U. (2011) A Study of the Thallium-and Bismuth-Based High-Temperature Superconductors in the Framework of the Generalized BCS Equations. Journal of Superconductivity and Novel Magnetism, 24, 255-260. 
http://dx.doi.org/10.1007/s10948-010-1009-0</mixed-citation></ref><ref id="scirp.58595-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. (2010) Generalized BCS Equations: Applications. International Journal of Modern Physics B, 24, 3701-3712. http://dx.doi.org/10.1142/S0217979210055858</mixed-citation></ref><ref id="scirp.58595-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P., Chávez, I. and de Llano, M. (2013) Generalized BCS Equations and Iron Pnictide Superconductors. Journal of Modern Physics, 4, 474-480. http://dx.doi.org/10.4236/jmp.2013.44067</mixed-citation></ref><ref id="scirp.58595-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Bednorz, J.G. and Müller, K.A. (1987) The New Approach to High-Tc Superconductivity. Nobel Lecture, 424-457.</mixed-citation></ref><ref id="scirp.58595-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. (2014) BCS-BEC Crossover without Appeal to Scattering Theory. International Journal of Modern Physics B, 28, Article ID: 1450054, 13 p. http://dx.doi.org/10.1142/S0217979214500544</mixed-citation></ref><ref id="scirp.58595-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. (2014) Towards a Solution of the Puzzle Posed by Superconducting SrTiO3. International Journal of Modern Physics B, 28, Article ID: 1450238, 14 p. http://dx.doi.org/10.1142/S0217979214502385</mixed-citation></ref><ref id="scirp.58595-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Le Tacon, M., et al. (2014) Inelastic X-ray Scattering in YBa2Cu3O6.6 Reveals Giant Phonon Anomalies and Elastic Central Peak Due to Charge-Density-Wave Formation. Nature Physics, 10, 52-58. http://dx.doi.org/10.1038/nphys2805</mixed-citation></ref><ref id="scirp.58595-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Sietz, F. (1940) The Modern Theory of Solids. McGraw-Hill, New York.</mixed-citation></ref><ref id="scirp.58595-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Poole Jr., C.P., Farach, H.A., Creswick, R.J. and Prozov, R. (2007) Handbook of Superconductivity. 2nd Edition, Academic Press, Amsterdam, 213.</mixed-citation></ref><ref id="scirp.58595-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Poole Jr., C.P., Farach, H.A., Creswick, R.J. and Prozov, R. (2007) Handbook of Superconductivity. 2nd Edition, Academic Press, Amsterdam, 87.</mixed-citation></ref><ref id="scirp.58595-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Berggold, K., Lorenz, T., Baier, J., Kriener, M., Senff, D., Roth, H., et al. (2006) Magnetic Heat Transport in R2CuO4 (R=La, Pr, Nd, Sm, Eu, and Gd). Physical Review B, 73, Article ID: 104430, 7 p. 
http://dx.doi.org/10.1103/PhysRevB.73.104430</mixed-citation></ref><ref id="scirp.58595-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Alexandrov, A.S. (2001) Nonadiabatic Superconductivity in MgB2 and Cuprates.  
http://arxiv.org/abs/cond-mat/0104413</mixed-citation></ref><ref id="scirp.58595-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Jarlborg, T. and Bianconi, A. (2013) Fermi Surface Reconstruction of Superoxygenated La2CuO4 Superconductors with Ordered Oxygen Interstitials. Physical Review B, 87, Article ID: 054514, 5 p. 
http://dx.doi.org/10.1103/PhysRevB.87.054514</mixed-citation></ref><ref id="scirp.58595-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Malik, G.P. and Malik, U. (2003) High-Tc Superconductivity via Superpropagators. Physica B: Condensed Matter, 336, 349-352. http://dx.doi.org/10.1016/S0921-4526(03)00302-8</mixed-citation></ref><ref id="scirp.58595-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Cracknell, A.P. and Kong, K.C. (1973) The Fermi Surface. Clarendon Press, Oxford.</mixed-citation></ref><ref id="scirp.58595-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">Suhl, H., Matthias, B.T. and Walker, L.R. (1959) Bardeen-Cooper-Schrieffer Theory of Superconductivity in the Case of Overlapping Bands. Physical Review Letters, 3, 552-554. http://dx.doi.org/10.1103/PhysRevLett.3.552</mixed-citation></ref><ref id="scirp.58595-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">Weinberg, S. (1972) Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity. John Wiley &amp; Sons Ltd., New York.</mixed-citation></ref></ref-list></back></article>