<?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">AMPC</journal-id><journal-title-group><journal-title>Advances in Materials Physics and Chemistry</journal-title></journal-title-group><issn pub-type="epub">2162-531X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ampc.2012.24037</article-id><article-id pub-id-type="publisher-id">AMPC-26019</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Chemistry&amp;Materials Science</subject><subject> Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Theory of Electron Density of States of High Temperature Impurity Induced Anharmonic Superconductors
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>empal</surname><given-names>Singh</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>Anu</surname><given-names>Singh</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>Vinod</surname><given-names>Ashokan</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>B.</surname><given-names>D. Indu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Physics, Texas A&amp;amp;M University, Education City, Doha, Qatar</addr-line></aff><aff id="aff1"><addr-line>Department of Physics, Indian Institute of Technology Roorkee, India</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>drbdindu@gmail.com(BDI)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>12</month><year>2012</year></pub-date><volume>02</volume><issue>04</issue><fpage>249</fpage><lpage>254</lpage><history><date date-type="received"><day>August</day>	<month>21,</month>	<year>2012</year></date><date date-type="rev-recd"><day>September</day>	<month>25,</month>	<year>2012</year>	</date><date date-type="accepted"><day>October</day>	<month>3,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   The expression for the electron density of states (EDOS) of high temperature superconductors (HTS) has been derived taking the disorder and anharmonicity effects as a central problem. This has been dealt with the help of double time thermodynamic Green’s function theory for electrons via a generalized Hamiltonian which consists of the contribution due to 1) unperturbed electrons; 2) unperturbed phonons; 3) isotopic impurities; 4) anharmonicities (no BCS type Hamiltonian has been taken up in the formulation); and 5) electron-phonon interactions. The renormalization effects and emergence of pairons appears as a unique feature of the theory and dependence of EDOS on impurity concentration and temperature has been discussed in details with special reference to the HTS.  
     
 
</p></abstract><kwd-group><kwd>Dyson’s Equation; Lehman Representation; Anharmonicity</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The discovery of HTS [<xref ref-type="bibr" rid="scirp.26019-ref1">1</xref>], excitingly opened up a new field of research in solid state physics experimentalists as well as theorists. The effect of anharmonicity, impurities as electron-phonon problem in HTS is least studied [2-5] due to its very complicated nature, because the unit cell of these compounds contain, beside two superconducting planes, the chain elements connected by bridge with plain through the apical oxygen ions . The interaction of electrons with anharmonic lattice vibrations is a longstanding problem that is not yet fully understood. The effects of anharmonicity on the electron-phonon problem and more specifically on superconductivity are relatively unknown. The present investigation deals with the impurity induced anharmonic phonon-electron problem, in which the contribution due to anharmonicities, isotropic impurities and interference has been dealt via an almost complete Hamiltonian. Having developed the electron Green’s function the expressions for energy spectrum and electron density of states have been obtained with few new features for the High temperature superconductors.</p></sec><sec id="s2"><title>2. Quantum Dynamics of Electrons</title><p>Let us consider the double-time thermodynamic electron retarded Green’s function [6,7]</p><disp-formula id="scirp.26019-formula141418"><label>(1)</label><graphic position="anchor" xlink:href="8-1510093\a31b4efb-b84a-45f8-8d38-4cb185d4832c.jpg"  xlink:type="simple"/></disp-formula><p>via an almost complete Hamiltonian [5-7]</p><disp-formula id="scirp.26019-formula141419"><label>(2)</label><graphic position="anchor" xlink:href="8-1510093\74a23ecb-9739-4291-84bc-59e9f7450526.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="8-1510093\9a8064f7-1716-4b99-a324-f28b3d2f0d66.jpg" />, <img src="8-1510093\ae762a00-f46d-4ad8-a3d3-0dd09bc11b04.jpg" />, <img src="8-1510093\2de0e71f-9031-4c22-b5ee-f6699b0760c1.jpg" />, <img src="8-1510093\750f6919-733d-4ae0-a5c1-11be59a19258.jpg" />and<img src="8-1510093\fcee36bd-dfa5-4a7a-baf6-b5f250d48e4b.jpg" />, respectively are unperturbed electron-, unperturbed phonon-, electronphonon-, anharmonic (upto quartic terms)-, and defect contributions to the Hamiltonian <img src="8-1510093\4d4eea18-bcba-4578-8ab2-db325d502845.jpg" /> and are expressible in the form [<xref ref-type="bibr" rid="scirp.26019-ref8">8</xref>]</p><p><img src="8-1510093\1c25a4ef-ece3-4947-8a70-6af56d592c0b.jpg" /></p><p><img src="8-1510093\0c9a9e19-cb41-4174-a770-b7a35b7e5259.jpg" /></p><p><img src="8-1510093\56fecee2-eb81-4926-b881-f6c5b149e056.jpg" /></p><p><img src="8-1510093\c16ca806-8b9a-403c-b6bd-1d61d88c600f.jpg" /></p><p><img src="8-1510093\9bd3548e-48ae-402a-9d15-acf52c40ad43.jpg" /></p><p>In the above equations <img src="8-1510093\89871c4b-274c-4a45-aecf-576a899cad1f.jpg" /> and <img src="8-1510093\f3da2d80-a972-406d-a52a-3f1ba96181ae.jpg" /> are the electron creation (annihilation) and phonon field and momentum operators, respectively. <img src="8-1510093\c9ce27aa-5caa-467f-a1bd-41c0c235779d.jpg" />(<img src="8-1510093\b8474bdf-1a70-40a3-9f4e-4aa2d5d774f8.jpg" />and <img src="8-1510093\eb425856-ae99-4623-a019-afaa1dc5af92.jpg" /> are phonon and electron wave vectors) and <img src="8-1510093\15305f26-0ba1-4364-94dc-4a2f3953be2a.jpg" /> stands for electron-phonon coupling coefficient.<img src="8-1510093\566df4bb-f03b-4416-baa2-ea2270d1a89f.jpg" />, <img src="8-1510093\1d4db069-17ed-466f-8e70-345a19e3f86f.jpg" />and <img src="8-1510093\afee8d68-ad5c-4093-a116-bb96f6dc36b6.jpg" /> are anharmonic coupling coefficients mass and force constant change parameters, respectively. Following the equation of motion technique [8-10] of quantum dynamics via Hamiltonian (2) and using Dyson’s equation approach we can obtain the Green’s function as</p><disp-formula id="scirp.26019-formula141420"><label>(3)</label><graphic position="anchor" xlink:href="8-1510093\c871f17b-19df-4a82-a23f-5c6bd85fb2b2.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="8-1510093\33bdf76b-ab8e-461a-8b41-327d796b34c1.jpg" /> and <img src="8-1510093\12c8d15b-93dc-4376-8dae-8e2eda8cd87f.jpg" /> are electron and pairon frequencies.</p><p>The excitation spectrum i.e. a response function can be expressed as</p><disp-formula id="scirp.26019-formula141421"><label>(4)</label><graphic position="anchor" xlink:href="8-1510093\f836098c-d2af-4cf7-8c7b-cf10a15f88f9.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="8-1510093\9d2ce016-aa2d-4ce9-aff8-d9b5ae25728a.jpg" /> and <img src="8-1510093\9c87424e-c9d4-4dbe-8a8a-c36c56c032c8.jpg" /> are the electron energy shift and electron line width respectively. Higher order Green’s function appearing in response function is decoupled using an appropriate decoupling scheme and the remaining Green’s function is evaluated via a renormalized electron and phonon Hamiltonian</p><p><img src="8-1510093\29e75b07-cd87-40ec-bd22-db96431681e4.jpg" /><img src="8-1510093\7acfb050-8953-4f01-af70-80cfbb5dbec8.jpg" /> (5)</p><disp-formula id="scirp.26019-formula141422"><label>(6)</label><graphic position="anchor" xlink:href="8-1510093\314c933a-78f0-4251-b7c3-e1a7538a70ee.jpg"  xlink:type="simple"/></disp-formula><p>Equation (3) can be written in simplified form as</p><disp-formula id="scirp.26019-formula141423"><label>(7)</label><graphic position="anchor" xlink:href="8-1510093\dd50565f-1e92-4c57-9ef5-de90b0b98065.jpg"  xlink:type="simple"/></disp-formula><p>with electron perturbed mode<img src="8-1510093\60024d4e-c05b-4c57-8b1a-6bf0d8b5cc1a.jpg" />and renormalized electron mode <img src="8-1510093\6c6be814-7387-41b0-a755-da3645987a94.jpg" />frequencies</p><disp-formula id="scirp.26019-formula141424"><label>(8)</label><graphic position="anchor" xlink:href="8-1510093\40746dcf-016c-464c-a088-cdef5437e4ef.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\e82dbb92-d493-4140-a916-7a3c39456be6.jpg" />&#160;&#160;</p><disp-formula id="scirp.26019-formula141425"><label>(9)</label><graphic position="anchor" xlink:href="8-1510093\e6313c5e-b79b-4776-9da5-84388193e204.jpg"  xlink:type="simple"/></disp-formula><p>Now electron energy shift and line widths are obtainable as</p><disp-formula id="scirp.26019-formula141426"><label>(10)</label><graphic position="anchor" xlink:href="8-1510093\c364fcfb-2e93-416c-90f3-e704e795672d.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\ffdc430d-70a6-4289-9732-4d72be57d8da.jpg" />&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141427"><label>(11)</label><graphic position="anchor" xlink:href="8-1510093\3d44971e-3aeb-43c7-bb62-80edd33dc039.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141428"><label>(12)</label><graphic position="anchor" xlink:href="8-1510093\b4fced93-f30e-4341-bf32-3c9c1739561b.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\40ff5519-0b9c-4012-973c-2c30df25784b.jpg" />&#160;&#160;</p><disp-formula id="scirp.26019-formula141429"><label>(13)</label><graphic position="anchor" xlink:href="8-1510093\e91ec223-ace5-46eb-9966-8e41e9d9f154.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\977f97b5-6ec0-4de6-aacb-9377c2481c7f.jpg" />&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141430"><label>(14)</label><graphic position="anchor" xlink:href="8-1510093\bebb99c5-9428-4e32-89a5-61930c3d4b57.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\1bfc1771-ed44-40e4-8c0c-e4421f3594e8.jpg" />&#160;</p><disp-formula id="scirp.26019-formula141431"><label>(15)</label><graphic position="anchor" xlink:href="8-1510093\9b70c35f-f300-4ad3-ac10-2d86a3cde213.jpg"  xlink:type="simple"/></disp-formula><p>where the superscript “D”, “3A”, “4A” and “ep” stand for the contributions due to defects, anharmonicities (cubic <img src="8-1510093\244f83e8-cd45-4738-8b43-62a4da0079de.jpg" /> and quartic<img src="8-1510093\1b717c82-c171-4c02-b370-57d44a187cb2.jpg" />) and electron-phonon interactions, respectively.</p><disp-formula id="scirp.26019-formula141432"><label>(16)</label><graphic position="anchor" xlink:href="8-1510093\cdf4af68-eda5-4cd2-9f96-7c91f97f7863.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141433"><label>(17)</label><graphic position="anchor" xlink:href="8-1510093\62195404-7b83-4f43-a88d-7f8198e8a0e6.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\89b87798-c4a0-42e0-9eae-3c340c936c48.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141434"><label>(18)</label><graphic position="anchor" xlink:href="8-1510093\44f90719-e391-48a0-a1b6-7c3c31df6191.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\a6843c59-4d92-4f0c-bc19-c86a3b6c3884.jpg" />&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141435"><label>(19)</label><graphic position="anchor" xlink:href="8-1510093\95f01b3a-7144-49eb-b252-6df372d29926.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141436"><label>(20)</label><graphic position="anchor" xlink:href="8-1510093\4c4b3685-aaa4-402f-9f0d-d8a80d0ab868.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141437"><label>(21)</label><graphic position="anchor" xlink:href="8-1510093\79a260b9-9689-45af-9982-426da83aa513.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Electron Density of States of High Temperature Superconductors</title><p>The electron density of states (EDOS) in Lehman representation can be expressed as</p><disp-formula id="scirp.26019-formula141438"><label>(22)</label><graphic position="anchor" xlink:href="8-1510093\c0187fcb-c4aa-457a-b1c7-038595a029df.jpg"  xlink:type="simple"/></disp-formula><p>Imaginary part of <img src="8-1510093\cb719bc5-f422-419e-a1bf-915980285ab7.jpg" /> is given by</p><disp-formula id="scirp.26019-formula141439"><label>(23)</label><graphic position="anchor" xlink:href="8-1510093\aa041570-5ead-4bd1-9fc8-9f39aeabc713.jpg"  xlink:type="simple"/></disp-formula><p>Using the imaginary part of Green’s function from Equation (23) in Equation (22) in Lehman representation we can write result&#160;</p><disp-formula id="scirp.26019-formula141440"><label>(24)</label><graphic position="anchor" xlink:href="8-1510093\05dd0e58-dd4a-4ff2-af94-c82dd29e6c61.jpg"  xlink:type="simple"/></disp-formula><p>Equation (24) can be reasonably approximated for small values of line width in the form</p><disp-formula id="scirp.26019-formula141441"><label>(25)</label><graphic position="anchor" xlink:href="8-1510093\319746bd-8f05-49fc-ba8a-0c9219083e83.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141442"><label>(26)</label><graphic position="anchor" xlink:href="8-1510093\48a32d61-a97c-4409-8084-425ebe01aaba.jpg"  xlink:type="simple"/></disp-formula><p>The various contributions to EDOS appears in Equation (26) can be summarized as</p><p><img src="8-1510093\e89963d5-4855-421f-af4b-4bd7600b6d3c.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141443"><label>(27)</label><graphic position="anchor" xlink:href="8-1510093\2a75a86b-9a60-471e-8b98-b1b7cc817ea0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141444"><label>(28)</label><graphic position="anchor" xlink:href="8-1510093\bf40522e-32a2-4495-9c79-aed0b2f93ce0.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141445"><label>(29)</label><graphic position="anchor" xlink:href="8-1510093\bf509cba-da16-4031-b345-180542d2c82a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141446"><label>(30)</label><graphic position="anchor" xlink:href="8-1510093\1f11a8a0-f048-4156-be32-1945019cb0d9.jpg"  xlink:type="simple"/></disp-formula><p>All the above expressions of density of states depend on the temperature. Let us examine EDOS in the following two regions.</p><p>Case-1 At the temperature very close to critical temperature, most of the electrons in superconducting state are paired. The collection of pairons (cooper pair, bipolarons) constitutes the condense or super fluid i.e. the pairons dominate over the normal electron<img src="8-1510093\0e0d422d-85ae-4c84-bb1c-03fe096ef594.jpg" /></p><p><img src="8-1510093\3528a769-b85c-4c55-a4f4-db35cc33a6de.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141447"><label>(31)</label><graphic position="anchor" xlink:href="8-1510093\6b043dc9-d5c2-4e15-9273-843f7360a1de.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\15357a56-8e68-425e-aae1-fc51a8361422.jpg" />&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141448"><label>(32)</label><graphic position="anchor" xlink:href="8-1510093\a517a480-bf74-4803-8488-543a78d14d89.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\0da5962d-0719-4d6e-b668-c96aa83a40d8.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;</p><disp-formula id="scirp.26019-formula141449"><label>(33)</label><graphic position="anchor" xlink:href="8-1510093\4924e93a-ed96-47ce-af00-b8b8fc5566d0.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\20844fd6-6e86-4702-a6ef-6b61298f29a7.jpg" />&#160;</p><disp-formula id="scirp.26019-formula141450"><label>(34)</label><graphic position="anchor" xlink:href="8-1510093\430e29f0-9b8d-487f-8f57-e36a3dd8fc27.jpg"  xlink:type="simple"/></disp-formula><p>Case-2 In this case <img src="8-1510093\90144133-ddca-4cba-a95d-a3a6b902bb68.jpg" /> , the contribution of normal energy becomes least than the pairon energy, so that the pairon energy dominates over the unpaired energy of the system and transits to the superconducting state. The EDOS in this situation becomes as</p><disp-formula id="scirp.26019-formula141451"><label>(35)</label><graphic position="anchor" xlink:href="8-1510093\ce2b251f-b2de-4fb7-aab0-6e8d8379ea93.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141452"><label>(36)</label><graphic position="anchor" xlink:href="8-1510093\a8055444-3ca1-4be4-9855-f57f3204c029.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141453"><label>(37)</label><graphic position="anchor" xlink:href="8-1510093\bb654e06-6270-4b6f-82e0-d5dbec4236fb.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141454"><label>(38)</label><graphic position="anchor" xlink:href="8-1510093\05f655fc-4a68-45a3-90bb-ec0ba1471c68.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141455"><label>(39)</label><graphic position="anchor" xlink:href="8-1510093\972d4fcd-60db-415d-91d1-9be106e7c6a8.jpg"  xlink:type="simple"/></disp-formula><p>The various symbols in above equations can be expressed as</p><disp-formula id="scirp.26019-formula141456"><label>(40)</label><graphic position="anchor" xlink:href="8-1510093\88e6a539-10bc-404c-97a1-a8ea86922a41.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141457"><label>(41)</label><graphic position="anchor" xlink:href="8-1510093\1c6612ef-3d13-4217-924a-5656f8436740.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141458"><label>(42)</label><graphic position="anchor" xlink:href="8-1510093\82a6e23a-4278-4bf8-9f46-b36424bfcfff.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.26019-formula141459"><label>(43)</label><graphic position="anchor" xlink:href="8-1510093\c4da6ef6-2237-41f5-a2ac-05618d089928.jpg"  xlink:type="simple"/></disp-formula><p><img src="8-1510093\365cb258-fd60-4912-9bf1-45f4089958b1.jpg" />is pairon distribution function.</p><p>Rest of the symbols are defined in references elsewhere [<xref ref-type="bibr" rid="scirp.26019-ref8">8</xref>].</p></sec><sec id="s4"><title>4. Results and Discussion</title><p>The variation of EDOS for <img src="8-1510093\8ee7f88d-caf5-45e8-8c04-33b62c8df144.jpg" /> and <img src="8-1510093\a63e3038-e0d3-43cb-acca-ba40575d59b0.jpg" /> is depicted in the Figures 1 and 2. These graphics are similar to the experimental imaging of quasi particle density of states for impurity induced <img src="8-1510093\f9f7594f-aa0c-4ec5-9120-c1a5cc9abe14.jpg" /> EDOS and anharmonic EDOS. The central peak in <xref ref-type="fig" rid="fig1">Figure 1</xref> exhibits the enhanced peak in the close vicinity of impurity site. This also reveals the evidence of four fold symmetric quasi particle cloud intensity peaks aligned with the nodes of the d-wave superconducting gap which is believed to characterize the HTSC and well supports the experimental observations of Pan et al. [11-12]. <xref ref-type="fig" rid="fig2">Figure 2</xref> describes the effects of cubic anharmonicities on electron density of states<img src="8-1510093\1addc481-4497-4269-8075-becae91d08dd.jpg" />. Four almost sharp peaks are found symmetrically distributed from both <img src="8-1510093\a98ad020-d014-4703-8d91-f99748c2ab5e.jpg" /> and <img src="8-1510093\7171e30d-ed44-42e2-9bad-3cd3dc384bf5.jpg" /> axes. It also notable that the pairon distribution function<img src="8-1510093\df014f2e-dc0b-4ba8-aded-6c08c417a806.jpg" />, energy <img src="8-1510093\d162bb3a-080e-426e-9521-4e2872e5b0a6.jpg" /> and temperature functions <img src="8-1510093\50ce2a5d-267f-432c-990e-42517725384f.jpg" /> heavily influence the anharmonic contribution to EDOS as well as the other terms appearing in the EDOS. It emerges from the present investigations that EDOS not only depends on energy but also on renormalized frequency, anharmonicities, impurity concentration and</p><p>temperature and well support to d-wave superconductivity.</p></sec><sec id="s5"><title>5. Acknowledgements</title><p>The authors (HS) and (AS) are thankful to Ministry of Human Resource development (MHRD), New Delhi and Council of Scientific and Industrial Research (CSIR), New Delhi for the financial support to carry out this research work.</p></sec><sec id="s6"><title>REFERENCES</title></sec><sec id="s7"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.26019-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">J. G. Bednorz and K. A. 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