<?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.2015.54032</article-id><article-id pub-id-type="publisher-id">WJCMP-61515</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>
 
 
  Coexistence of Spin Density Wave (SDW) and Superconductivity in Ba&lt;sub&gt;1-x&lt;/sub&gt;K&lt;sub&gt;x&lt;/sub&gt;Fe&lt;sub&gt;2&lt;/sub&gt;As&lt;sub&gt;2&lt;/sub&gt;
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>aftu</surname><given-names>Brhane</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Department of Physics, Haramaya University, Diredawa, Ethiopia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>haftuberhane@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>12</day><month>10</month><year>2015</year></pub-date><volume>05</volume><issue>04</issue><fpage>319</fpage><lpage>331</lpage><history><date date-type="received"><day>28</day>	<month>March</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>24</month>	<year>November</year>	</date><date date-type="accepted"><day>27</day>	<month>November</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>
 
 
  With the use of a model Hamiltonian and retarded double time green’s function formalism, we obtain mathematical expressions for spin density wave and superconductivity parameters. The model reveals a distinct possibility of the coexistence of magnetic phase and superconductivity, which are two usually irreconcilable cooperative phenomena. The work is motivated by the recent experimental evidences of coexistence of spin density wave and superconductivity in a number of FeAs-based superconductors. The theoretical results are then applied to show the coexistence of spin density wave and superconductivity in iron pnictide compound Ba
  <sub>1-x</sub>K
  <sub>x</sub>Fe
  <sub>2</sub>As
  <sub>2</sub> (0.2 ≤ x &lt; 0.4).
 
</p></abstract><kwd-group><kwd>Retarded Double Time Green’s Function Formalism</kwd><kwd> Spin Singlet and Triplet State</kwd><kwd> Spin Density Wave and Superconducting</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The interplay between superconductivity and magnetism has been an interesting topic in condensed mater physics which has been considered until very recently hostile and incompatible. Since the discovery of superconductivity in quaternary pnictide-oxides with critical temperatures (T<sub>C</sub>) up to 55 K a lot of tremendous interest has been generated in the study of coexistence of these two cooperative phenomena of superconductivity and magnetism. After first reports on superconductivity in undoped LaNiPO [<xref ref-type="bibr" rid="scirp.61515-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.61515-ref2">2</xref>] below 5 K, shortly after this discovery the breakthrough was a T<sub>C</sub> of 26 K in the F-doped arsenide LaO<sub>1</sub><sub>−</sub><sub>x</sub>F<sub>x</sub>FeAs system [<xref ref-type="bibr" rid="scirp.61515-ref3">3</xref>] .</p><p>In addition to this several groups reported an increase of T<sub>C</sub> values by replacing La with smaller-size rare- earth ions like CeO<sub>1</sub><sub>−x</sub>F<sub>x</sub>FeAs [<xref ref-type="bibr" rid="scirp.61515-ref4">4</xref>] , and samarium-arsenide oxides Sm(O<sub>1−x</sub>F<sub>x</sub>)FeAs with a critical temperature T<sub>C</sub> of 55 K [<xref ref-type="bibr" rid="scirp.61515-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.61515-ref6">6</xref>] . The iron based superconductors promise interesting applications. While the interplay of superconductivity and magnetism, as well as their mechanisms remains the issues of active debates and studies, one thing in FeSC riddle is clear that it is the complex multi-band electronic structure of these compounds that determine their rich and puzzling properties. What is important and captivating is that this complexity seems to play a positive role in the struggle for understanding the FeSC physics and also for search of the materials with higher T<sub>C</sub> [<xref ref-type="bibr" rid="scirp.61515-ref7">7</xref>] .</p><p>The FeSC is quite promising for applications. Having much higher Hc than cuprates and high isotropic critical currents [<xref ref-type="bibr" rid="scirp.61515-ref8">8</xref>] they are attractive for electrical power and magnet applications, while the coexistence of magnetism and superconductivity makes them interesting for spintronics [<xref ref-type="bibr" rid="scirp.61515-ref9">9</xref>] . All the compounds share similar electronic band structure in which the electronic states at the Fermi level are occupied predominantly by the Fe 3d electrons [<xref ref-type="bibr" rid="scirp.61515-ref7">7</xref>] .</p><p>By combining transport, X-ray and neutron diffraction experiment studies, the first member of a new family of iron pnictide superconductors (Ba<sub>1</sub><sub>−</sub><sub>x</sub>K<sub>x</sub>)Fe<sub>2</sub>As<sub>2</sub> with the ThCr<sub>2</sub>Si<sub>2</sub>-type structure was discovered a bulk superconductor with T<sub>C</sub> = 38 K and both the SDW and the superconducting orders coexist in the (Ba<sub>1</sub><sub>−</sub><sub>x</sub>K<sub>x</sub>)Fe<sub>2</sub>As<sub>2</sub> (0.2 ≤ x &lt; 0.4). The structural and electronic properties of the parent compound BaFe<sub>2</sub>As<sub>2</sub> are closely related to LaFeAsO. The induced superconductivity by hole doping is found to have a significantly higher TC in comparison with hole doped LaFeAsO. In contrast to previously stated opinions, the results prove that hole doping is definitely a possible pathway to induce high-T<sub>C</sub> superconductivity, at least in the oxygen-free compounds [<xref ref-type="bibr" rid="scirp.61515-ref10">10</xref>] .</p><p>The above exciting discovery stimulated a lot of interest in the study of coexistence of superconductivity and magnetism. The proximity of the magnetic and superconducting (SC) phases suggests a close relationship between the two phenomena. It is generally believed that the magnetic couplings between the itinerant electrons and/or between the itinerant electron and local spin are essential to both spin density wave instability and superconductivity. Besides, other experimental and theoretical findings, especially the antiferromagnetic ground state and the SDW anomaly of LaFeAsO strongly suggest that the pairing mechanism of the electrons is likely to be connected with spin fluctuations, as it has been assumed for the cuprates [<xref ref-type="bibr" rid="scirp.61515-ref10">10</xref>] .</p><p>Triplet superconductivity appears provided that we have coexistence of singlet superconductivity and SDW. In many high <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x6.png" xlink:type="simple"/></inline-formula> superconductors, superconducting mechanism is attributed to strong coulomb interactions of the electrons in the system, which can also be the cause for the appearance of SDW state. This suggests the existence of competition between the two states [<xref ref-type="bibr" rid="scirp.61515-ref11">11</xref>] . The properties of the unconventional triplet superconductivity and SDW with an emphasis on the analysis of their order parameter were reviewed.</p><p>Research on superconducting iron arsenides has largely focused on ternary compounds with the ThCr<sub>2</sub>Si<sub>2</sub>-type structure, rather than arsenide oxides (LaFeAsO derivatives) [<xref ref-type="bibr" rid="scirp.61515-ref12">12</xref>] . This is because single-phase samples and also large single crystals of the ternary compounds are much easier to obtain. Partial replacement of barium for potassium (hole doping) induced superconductivity at 38 K in (Ba<sub>0.6</sub>K<sub>0.4</sub>)Fe<sub>2</sub>As<sub>2</sub>, [<xref ref-type="bibr" rid="scirp.61515-ref13">13</xref>] .</p><p>The relation between the spin-density-wave (SDW) and superconducting order is a central topic in current research on the superconducting iron pnictide based high TC superconductors. So, in this paper, we start with a model Hamiltonian which incorporates not only terms of the BCS but also by assuming the pairing interaction is due to spin fluctuations for iron pnictide superconductors Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub>, to examine the coexistence of spin density wave and superconductivity.</p></sec><sec id="s2"><title>2. Model Hamiltonian of the System</title><p>The purpose of this work is to study theoretically the co-existence of spin density wave and superconductivity properties in the compound Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub> in general and to find expression for transition temperature and order parameter in particular. For this purpose, we tried to find the mathematical expression for the superconducting critical temperature (T<sub>C</sub>), superconducting order parameter (∆<sub>sc</sub>) the magnetic order parameter (M) and SDW transition temperature (T<sub>SDW</sub>). Within the framework of the BCS model, the model of the Hamiltonian for coexistence SDW and superconductivity in the compound can be express as:</p><disp-formula id="scirp.61515-formula1744"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x7.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x8.png" xlink:type="simple"/></inline-formula> are the creation (annihilation) operators of an electron having the wave number p and spin<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x9.png" xlink:type="simple"/></inline-formula>.</p><p>Whereas (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x10.png" xlink:type="simple"/></inline-formula>) superconducting order parameter and (M) SDW order parameters. The Hamiltonian in (1) will be used to determine the equations of motion in terms of the Green function.</p><sec id="s2_1"><title>2.1. Coupling of SDW and Superconducting Order Parameters</title><p>The Double time dependent Green’s function equal to the change of the average value of some dynamic quantity by the time t and useful because they can be used to describe the effect of retarded interactions and all quantities of physical interest can be derived from them. To get the equation of motion we use the double-time temperature dependent retarded Green function is given by Zubarev [<xref ref-type="bibr" rid="scirp.61515-ref14">14</xref>] :</p><disp-formula id="scirp.61515-formula1745"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x11.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x12.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x13.png" xlink:type="simple"/></inline-formula> are Heisenberg operators and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x14.png" xlink:type="simple"/></inline-formula> is the Heaviside step function. Now, using Dirac delta function and Heisenberg operators, we can write as:</p><disp-formula id="scirp.61515-formula1746"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x15.png"  xlink:type="simple"/></disp-formula><p>The Fourier transformation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x16.png" xlink:type="simple"/></inline-formula> is given by</p><disp-formula id="scirp.61515-formula1747"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x17.png"  xlink:type="simple"/></disp-formula><p>Taking the Fourier transform we get:</p><disp-formula id="scirp.61515-formula1748"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x18.png"  xlink:type="simple"/></disp-formula><p>From (4), it follows that</p><disp-formula id="scirp.61515-formula1749"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x19.png"  xlink:type="simple"/></disp-formula><p>where the anti-commutation relation,</p><disp-formula id="scirp.61515-formula1750"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x20.png"  xlink:type="simple"/></disp-formula><p>has been used. To derive an expression for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x21.png" xlink:type="simple"/></inline-formula>, we have calculate the commutator<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x22.png" xlink:type="simple"/></inline-formula>, using</p><p>(1) and using the identities and</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x23.png" xlink:type="simple"/></inline-formula>and (7)</p><p>Solving the commutator in Equation (5) by using the Hamiltonian in e Equation (1), we get</p><disp-formula id="scirp.61515-formula1751"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x25.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1752"><label>(8a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x26.png"  xlink:type="simple"/></disp-formula><p>After some lengthy but straightforward calculations; we arrive at the following results:</p><disp-formula id="scirp.61515-formula1753"><label>(8b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x27.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1754"><label>(8c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x28.png"  xlink:type="simple"/></disp-formula><p>Substituting (8) in to (5), we get</p><disp-formula id="scirp.61515-formula1755"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x29.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1756"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x30.png"  xlink:type="simple"/></disp-formula><p>The equation of motion for the correlation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x31.png" xlink:type="simple"/></inline-formula> in (9) can be described as:</p><disp-formula id="scirp.61515-formula1757"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x32.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1758"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x33.png"  xlink:type="simple"/></disp-formula><p>Evaluating the commutator in Equation (10) using Hamiltonian:</p><disp-formula id="scirp.61515-formula1759"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x34.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1760"><label>(11a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x35.png"  xlink:type="simple"/></disp-formula><p>After some lengthy but straightforward calculations; we arrive at the following results:</p><disp-formula id="scirp.61515-formula1761"><label>(11b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x36.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1762"><label>(11c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x37.png"  xlink:type="simple"/></disp-formula><p>Substituting (11) in to (10), we get</p><disp-formula id="scirp.61515-formula1763"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x38.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1764"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x39.png"  xlink:type="simple"/></disp-formula><p>Similarly as we did in the above the equation of motion for the correlation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x40.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x41.png" xlink:type="simple"/></inline-formula></p><p>is given by:</p><disp-formula id="scirp.61515-formula1765"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x42.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1766"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x43.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.61515-formula1767"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x44.png"  xlink:type="simple"/></disp-formula><p>From Equation (12), we obtain:</p><disp-formula id="scirp.61515-formula1768"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x45.png"  xlink:type="simple"/></disp-formula><p>And from Equation (14):</p><disp-formula id="scirp.61515-formula1769"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x46.png"  xlink:type="simple"/></disp-formula><p>Plugging Equations (15) and (16) in (9), yields:</p><disp-formula id="scirp.61515-formula1770"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x47.png"  xlink:type="simple"/></disp-formula><p>And insert Equations (15) and (16) in (13), we have:</p><disp-formula id="scirp.61515-formula1771"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x48.png"  xlink:type="simple"/></disp-formula><p>Applying nesting condition<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x49.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x50.png" xlink:type="simple"/></inline-formula>and use approximation,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x51.png" xlink:type="simple"/></inline-formula>; Equations (17) and (14) becomes:</p><disp-formula id="scirp.61515-formula1772"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x52.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.61515-formula1773"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x53.png"  xlink:type="simple"/></disp-formula><p>Let <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x54.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x55.png" xlink:type="simple"/></inline-formula></p><p>Then Equations (19) and (20) respectively becomes:</p><disp-formula id="scirp.61515-formula1774"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x56.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1775"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x57.png"  xlink:type="simple"/></disp-formula><p>Finally we can express:</p><disp-formula id="scirp.61515-formula1776"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x58.png"  xlink:type="simple"/></disp-formula><p>Using the expression<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x59.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x59.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x60.png" xlink:type="simple"/></inline-formula> is effective order parameter and the Matsubara’s frequency, we can write Equation (23) as:</p><disp-formula id="scirp.61515-formula1777"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x61.png"  xlink:type="simple"/></disp-formula><p>To take into account the temperature dependence of order parameters, we shall write as:</p><disp-formula id="scirp.61515-formula1778"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x62.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1779"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x63.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x64.png" xlink:type="simple"/></inline-formula></p><p>Using Equation (24) into Equation (25), we obtain</p><disp-formula id="scirp.61515-formula1780"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x65.png"  xlink:type="simple"/></disp-formula><p>Let us use</p><disp-formula id="scirp.61515-formula1781"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x66.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.61515-formula1782"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x67.png"  xlink:type="simple"/></disp-formula><p>Plugging Equation (28) and Equation (29) in Equation (27), we get:</p><disp-formula id="scirp.61515-formula1783"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x68.png"  xlink:type="simple"/></disp-formula><p>For mathematical convenience, we replace the summation in (27) by integration. Thus</p><disp-formula id="scirp.61515-formula1784"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x69.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x70.png" xlink:type="simple"/></inline-formula> is the density of states at the Fermi level.</p><p>The density of state <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x71.png" xlink:type="simple"/></inline-formula></p><p>Assume <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x72.png" xlink:type="simple"/></inline-formula> this implies that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x73.png" xlink:type="simple"/></inline-formula>. For j = 2:</p><disp-formula id="scirp.61515-formula1785"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x74.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x75.png" xlink:type="simple"/></inline-formula></p><p>Finally we can write Equation (31) as:</p><disp-formula id="scirp.61515-formula1786"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x76.png"  xlink:type="simple"/></disp-formula><p>From (32), it clearly follows that the order parameters <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x77.png" xlink:type="simple"/></inline-formula> and M, for superconductivity and SDW are interdependent.</p><p>We now consider the equations of motion for SDW, we can write,</p><disp-formula id="scirp.61515-formula1787"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x78.png"  xlink:type="simple"/></disp-formula><p>Doing a lot as we did in the above, we finally get:</p><disp-formula id="scirp.61515-formula1788"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x79.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1789"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x80.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1790"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x81.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.61515-formula1791"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x82.png"  xlink:type="simple"/></disp-formula><p>Doing a lot as we did in the previous, we finally get:</p><disp-formula id="scirp.61515-formula1792"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x83.png"  xlink:type="simple"/></disp-formula><p>Using Equation (38) in to Equation (26), the SDW order Parameter M is given by:</p><disp-formula id="scirp.61515-formula1793"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x84.png"  xlink:type="simple"/></disp-formula><p>or</p><disp-formula id="scirp.61515-formula1794"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x85.png"  xlink:type="simple"/></disp-formula><p>So, finally we get:</p><disp-formula id="scirp.61515-formula1795"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x86.png"  xlink:type="simple"/></disp-formula><p>From (41), it is again evident that the order parameters <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x87.png" xlink:type="simple"/></inline-formula> and M, for superconductivity and SDW are interdependent, as was the case from (32).</p><p>It is, therefore, possible that in some temperature interval, SDW and superconductivity can co-exist, although one phase has a tendency to suppress the critical temperature and the order parameter of the other phase.</p></sec><sec id="s2_2"><title>2.2. Dependence of the Magnetic Order Parameter on the Transition Temperature for Spin Density Wave and Superconductivity</title><p>To study Equation (32), we consider the case, when <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x88.png" xlink:type="simple"/></inline-formula></p><p>We can then replace</p><disp-formula id="scirp.61515-formula1796"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x89.png"  xlink:type="simple"/></disp-formula><p>In (32) and get,</p><disp-formula id="scirp.61515-formula1797"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x90.png"  xlink:type="simple"/></disp-formula><p>Using the integral relation,</p><disp-formula id="scirp.61515-formula1798"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x91.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1799"><label>(42)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x92.png"  xlink:type="simple"/></disp-formula><p>the above equation reduces to,</p><disp-formula id="scirp.61515-formula1800"><label>(43)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x93.png"  xlink:type="simple"/></disp-formula><p>from the BCS theory, the order parameter<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x94.png" xlink:type="simple"/></inline-formula>, at T = 0 for a given superconductor with transition temperature T<sub>C</sub> is given by</p><disp-formula id="scirp.61515-formula1801"><label>(44)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x95.png"  xlink:type="simple"/></disp-formula><p>using this result in (43), we obtain</p><disp-formula id="scirp.61515-formula1802"><label>(45)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x96.png"  xlink:type="simple"/></disp-formula><p>To solve (45) numerically we use Debay temperature and the interband BCS coupling constant.</p><p>To estimate α, I consider the case <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x97.png" xlink:type="simple"/></inline-formula> which implies, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x98.png" xlink:type="simple"/></inline-formula></p><p>From (32), we then have</p><disp-formula id="scirp.61515-formula1803"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x99.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1804"><label>(46)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x100.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1805"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x101.png"  xlink:type="simple"/></disp-formula><p>Putting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x102.png" xlink:type="simple"/></inline-formula> and for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x102.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x103.png" xlink:type="simple"/></inline-formula> we can write</p><disp-formula id="scirp.61515-formula1806"><label>(47)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x104.png"  xlink:type="simple"/></disp-formula><p>Using Laplacian’s transformation with Matsuber relation result we can write,</p><disp-formula id="scirp.61515-formula1807"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x105.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x106.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x106.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x107.png" xlink:type="simple"/></inline-formula> and using integrating by part,</p><disp-formula id="scirp.61515-formula1808"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x108.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1809"><label>(48)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x109.png"  xlink:type="simple"/></disp-formula><p>Using the fact that, for low temperature, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x110.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x110.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x111.png" xlink:type="simple"/></inline-formula> is the Euler constant having the value</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x112.png" xlink:type="simple"/></inline-formula>(Hsian) [<xref ref-type="bibr" rid="scirp.61515-ref15">15</xref>] and the last equation can be neglected since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x113.png" xlink:type="simple"/></inline-formula> is very small.</p><p>We can write (48) as,</p><disp-formula id="scirp.61515-formula1810"><label>(49)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x114.png"  xlink:type="simple"/></disp-formula><p>Using L’Hospital’s rule, it is easy to show that</p><disp-formula id="scirp.61515-formula1811"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x115.png"  xlink:type="simple"/></disp-formula><p>which can be neglected since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x116.png" xlink:type="simple"/></inline-formula> is very small.</p><p>Substituting (49) in (46), we then obtain</p><disp-formula id="scirp.61515-formula1812"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x117.png"  xlink:type="simple"/></disp-formula><p>This implies,</p><disp-formula id="scirp.61515-formula1813"><label>(50)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x118.png"  xlink:type="simple"/></disp-formula><p>which can be used to estimate <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x119.png" xlink:type="simple"/></inline-formula> for Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub>, using the experimental value <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x119.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x120.png" xlink:type="simple"/></inline-formula> and cut-off</p><p>energy.</p><p>To study how M depends on the magnetic transition temperature<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x121.png" xlink:type="simple"/></inline-formula>, we consider (41).</p><disp-formula id="scirp.61515-formula1814"><label>(51)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x122.png"  xlink:type="simple"/></disp-formula><p>proceeding as before, it is easy to show that,</p><disp-formula id="scirp.61515-formula1815"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x123.png"  xlink:type="simple"/></disp-formula><p>Neglecting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x124.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.61515-formula1816"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x125.png"  xlink:type="simple"/></disp-formula><p>This gives;</p><disp-formula id="scirp.61515-formula1817"><label>(52)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x126.png"  xlink:type="simple"/></disp-formula><p>we can use (52) to draw the phase diagram for M and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x127.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_3"><title>2.3. Pairing of Spin Density Wave (SDW) and Triplet Superconductivity</title><p>In this section we want to drive an expressions for the order parameters of SDW, M, and triplet superconductivity, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x128.png" xlink:type="simple"/></inline-formula>, as a function of both of them and temperature, and to compare the variation of each with temperature. Still we can use the Hamiltonian given by Equation (1), but in this case the superconducting order parameter depends on spin alignment [<xref ref-type="bibr" rid="scirp.61515-ref16">16</xref>] and they can be expressed as;</p><disp-formula id="scirp.61515-formula1818"><label>(53)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x129.png"  xlink:type="simple"/></disp-formula><p>where the superconducting order parameter is given by:</p><disp-formula id="scirp.61515-formula1819"><label>(54)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x130.png"  xlink:type="simple"/></disp-formula><p>We now consider the equation of motion:</p><disp-formula id="scirp.61515-formula1820"><label>(55)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x131.png"  xlink:type="simple"/></disp-formula><p>Doing a lot as we did in the above for the commutation and using the assumption <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x132.png" xlink:type="simple"/></inline-formula> we finally get:</p><disp-formula id="scirp.61515-formula1821"><label>(56)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x133.png"  xlink:type="simple"/></disp-formula><p>The nesting property of the Fermi surface that expected for low dimensional band structure and attributed to the SDW ordering gives as an expression<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x134.png" xlink:type="simple"/></inline-formula>.</p><p>Finally:</p><disp-formula id="scirp.61515-formula1822"><label>(57)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x135.png"  xlink:type="simple"/></disp-formula><p>Since we are dealing with only the triplet pair; we can ignore the singlet correlation.</p><p>The equation of motion for correlation in RHS of (57) is written as:</p><disp-formula id="scirp.61515-formula1823"><label>(58)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x136.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.61515-formula1824"><label>(59)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x137.png"  xlink:type="simple"/></disp-formula><p>which can be rewritten, after solving the commutation relation and removing the singlet pair.</p><p>From Equations (58) and (59), we will get;</p><disp-formula id="scirp.61515-formula1825"><label>(60)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x138.png"  xlink:type="simple"/></disp-formula><p>With help of Equation (60) and Equation (57):</p><disp-formula id="scirp.61515-formula1826"><label>(61)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x139.png"  xlink:type="simple"/></disp-formula><p>which in turn can be written as:</p><disp-formula id="scirp.61515-formula1827"><label>(62)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x140.png"  xlink:type="simple"/></disp-formula><p>Applying nesting condition<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x141.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x142.png" xlink:type="simple"/></inline-formula>and use approximation,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x141.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x142.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x143.png" xlink:type="simple"/></inline-formula>; Equation (62) becomes:</p><disp-formula id="scirp.61515-formula1828"><label>(63)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x144.png"  xlink:type="simple"/></disp-formula><p>Using the expression<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x145.png" xlink:type="simple"/></inline-formula>, Equation (29) and Matsubara’s frequency, we can write Equation (63) as:</p><disp-formula id="scirp.61515-formula1829"><label>(64)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x146.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.61515-formula1830"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x147.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.61515-formula1831"><graphic  xlink:href="http://html.scirp.org/file/7-4800290x148.png"  xlink:type="simple"/></disp-formula><p>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800290x149.png" xlink:type="simple"/></inline-formula></p><p>By taking an approximation over the superconducting order parameter, such that it is independent of wave vector, finally we get:</p><disp-formula id="scirp.61515-formula1832"><label>(65)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x150.png"  xlink:type="simple"/></disp-formula><p>We now consider the equations of motion for SDW, we can write,</p><disp-formula id="scirp.61515-formula1833"><label>(66)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x151.png"  xlink:type="simple"/></disp-formula><p>Doing a lot as we did in the above, we finally get:</p><disp-formula id="scirp.61515-formula1834"><label>(67)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x152.png"  xlink:type="simple"/></disp-formula><p>So,</p><disp-formula id="scirp.61515-formula1835"><label>(68)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800290x153.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s3"><title>3. Results</title><p>Starting with a model Hamiltonian for the system and using Green’s function formalism, we obtained expressions for superconducting transition temperature (T<sub>C</sub>), magnetic order parameter (M) and spin density wave transition temperature (T<sub>SDW</sub>). Based on these result we found two very vital equations ((45) and (52)). Moreover, we scrutinized the effect of magnetic order parameter (M) on superconducting transition temperature (T<sub>C</sub>) and spin density wave transition temperature (T<sub>SDW</sub>) in Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub> by using the relevant parameters. For this purpose, we have used (45) which have been numerically solved using the relevant parameters to plot the phase diagram for magnetic order parameter (M) versus superconducting transition temperature (T<sub>C</sub>). In the same figure, we have also plotted the phase diagram of magnetic ordering (M) versus spin density wave transition temperature (T<sub>SDW</sub>), using (52). From the graph we observe T<sub>C</sub> decreases with increase in M, whereas T<sub>SDW</sub> increases with increase in M. The phase diagrams of M versus T<sub>C</sub> and M versus T<sub>SDW</sub>, were merged to obtain the region where both spin density wave and superconductivity co-exist. The regions of intersection of the two merged graphs showed in <xref ref-type="fig" rid="fig1">Figure 1</xref> indicate co-existence of spin density wave and superconductivity for Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub>.</p></sec><sec id="s4"><title>4. Conclusion</title><p>Using a model Hamiltonian consisting of spin density wave and superconducting part and applying Green’s function formalism we have got an expression which shows the relation of the two order parameters and their variation with temperature. From <xref ref-type="fig" rid="fig1">Figure 1</xref> we observe that T<sub>C</sub> decreases with increase in M, whereas T<sub>SDW</sub> increases with increase in M. The spin density wave and superconducting phases, therefore, resist each other. However, the present work shows that there is a small region of temperature, where both the phases may be in existence together, which is indicated by (SC + SDW) in the figure. In the absence of spin density wave the expression for both singlet and triplet cases reduces to the well known BCS result. My study explicitly shows that</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Co-existence of spin density wave (SDW) and superconductivity in Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub></title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-4800290x154.png"/></fig><p>spin density wave and superconductivity truly coexist in Ba<sub>1−x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub> (0.2 ≤ x &lt; 0.4) in some range of magnetic order.</p></sec><sec id="s5"><title>Acknowledgements</title><p>I thank Prof. Amarendra Rajput for providing me constructive comments, suggestions and valuable support.</p></sec><sec id="s6"><title>Cite this paper</title><p>HaftuBrhane, (2015) Coexistence of Spin Density Wave (SDW) and Superconductivity in Ba<sub>1-x</sub>K<sub>x</sub>Fe<sub>2</sub>As<sub>2</sub>. 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