<?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.2015.53013</article-id><article-id pub-id-type="publisher-id">WJCMP-58321</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>
 
 
  Study of Upper Critical Magnetic Field of Superconducting HoMo&lt;sub&gt;6&lt;/sub&gt;Se&lt;sub&gt;8&lt;/sub&gt;
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>adesse</surname><given-names>Desta</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>Pooran</surname><given-names>Singh</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>Gebregziabher</surname><given-names>Kahsay</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="aff1"><addr-line>Department of Physics, College of Natural Science, Addis Ababa University, Addis Ababa, Ethiopia</addr-line></aff><aff id="aff2"><addr-line>Department of Physics, College of Science, Bahir Dar University, Bahir Dar, Ethiopia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>tad4jju@gmail.com(AD)</email>;<email>psinghgbpup@yahoo.com(PS)</email>;<email>michige_90@yahoo.com(GK)</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>105</fpage><lpage>117</lpage><history><date date-type="received"><day>25</day>	<month>April</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>24</month>	<year>July</year>	</date><date date-type="accepted"><day>27</day>	<month>July</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>
 
 
  This work focuses on the study of mathematical aspects of upper critical magnetic field of superconducting HoMo
  <sub>6</sub>Se
  <sub>8</sub>. At zero external magnetic field, HoMo
  <sub>6</sub>Se
  <sub>8</sub> was found to undergo a transition from the normal state to the superconducting state at 5.6 K and returned to a normal but magnetically ordered state between the temperature range of 0.3 K and 0.53 K. The main objective of this work is to show the temperature dependence of the upper critical magnetic field of superconducting HoMo
  <sub>6</sub>Se
  <sub>8</sub> by using the Ginzburg-Landau (GL) phenomenological Equation. We found the direct relationship between the GL coherence length (
  <em>ξ</em>
  <sub><em>GL</em></sub>) and penetration depth (
  <em>λ</em>
  <sub>GL</sub>) with temperature. From the GL Equations and the results obtained for the GL coherence length, the expression for upper critical magnetic field (
  <em>H</em>
  <sub><em>c2</em></sub>) is obtained for the superconducting HoMo
  <sub>6</sub>Se
  <sub>8</sub>. The result is plotted as a function of temperature. The graph shows the linear dependence of upper critical magnetic field (
  <em>H</em>
  <sub><em>c2</em></sub>) with temperature (T) and our finding is in agreement with experimental observations.
 
</p></abstract><kwd-group><kwd>Ginzburg-Landau Equation</kwd><kwd> Upper Critical Magnetic Field</kwd><kwd> HoMo&lt;sub&gt;6&lt;/sub&gt;Se&lt;sub&gt;8&lt;/sub&gt;</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Superconductivity is a phenomenon that occurs at very low temperatures. Every superconductor has a transition temperature (T<sub>c</sub>) below which it superconducts and above which it is a normal metal [<xref ref-type="bibr" rid="scirp.58321-ref1">1</xref>] . In the superconducting state, the material has no electrical resistance and thus conducts electricity without losses. On the other hand, in the normal state, the material does have resistance and the flow of electric current accompanies with the development of heat and the dissipation of energy [<xref ref-type="bibr" rid="scirp.58321-ref1">1</xref>] .</p><p>The era of low-temperature physics began in 1908 when the Dutch physicist Heike Kamerlingh Onnes first liquefied helium which boiled at 4.2 K at standard pressure. Three years later, in 1911, Kamerlingh Onnes discovered the phenomenon of superconductivity while studying the resistivity of metals at low temperatures [<xref ref-type="bibr" rid="scirp.58321-ref1">1</xref>] .</p><p>Most of the fundamental properties of superconductors vary from material to material. The superconducting state, as any state of matter, has its own basic properties. So, any superconductor independent of the mechanism of superconductivity and the material will exhibit these properties. The basic properties of the superconducting state are zero resistance, Meissner effect, magnetic flux quantization, Josephson effects, the BCS theory, Cooper pair, appearance of an energy gap in elementary excitation energy spectrum, Isotope effect and the proximity effect. Every superconducting transition is marked by a jump in specific heat. In the mixed state, the behavior of type-II superconductors has the same pattern [<xref ref-type="bibr" rid="scirp.58321-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref4">4</xref>] .</p><p>HoMo<sub>6</sub>Se<sub>8</sub> compound is building blocks of the Chevrel-phase crystal structure [<xref ref-type="bibr" rid="scirp.58321-ref5">5</xref>] . The discovery in 1984 of the new superconducting HoMo<sub>6</sub>Se<sub>8</sub> gave rise to a renewed interest in the interplay of magnetism and superconductivity. From the experimental results, a magnetic phase transition (T<sub>n</sub> = 0.53 K) to a long-period magnetic states has been observed via neutron scattering in the superconductor HoMo<sub>6</sub>Se<sub>8</sub> (T<sub>c</sub> = 5.6 K) [<xref ref-type="bibr" rid="scirp.58321-ref6">6</xref>] . The characteristic wave vector (q<sub>c</sub>) is strongly temperature dependent and there is no observation of higher-order satellites.</p><p>The rare occurrence of ferromagnetism, as found in HoMo<sub>6</sub>Se<sub>8</sub> and HoMo<sub>6</sub>Se<sub>8</sub>, revealed the strongly competitive nature of these two cooperative phenomena in the form of long-wavelength at low oscillatory magnetic temperature (&lt;1 K) and a ferromagnetic lock-in transition that quenched the superconductivity. No sign of reentrant behavior (in zero field) was observed down to 0.04 K [<xref ref-type="bibr" rid="scirp.58321-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref7">7</xref>] . Ternary rare-earth superconductors which display a propensity for ferromagnetism have received considerable experimental as well as theoretical attention recently. In the case of the new superconductors, HoMo<sub>6</sub>Se<sub>8</sub> was observed despite the presence of the holmium moment of the rare earth ion in each unit cell. These compounds did not destroy the property of superconductivity at low temperature. In HoMo<sub>6</sub>Se<sub>8</sub>, the domain coexistence phase survives till T = 0.3 K (the exchange interaction is weaker and the coexistence persists down to T = 0.3 K) [<xref ref-type="bibr" rid="scirp.58321-ref8">8</xref>] . In addition to the superconducting and ferromagnetic domains, a coexistence region is observed in HoMo<sub>6</sub>Se<sub>8</sub> in which the superconducting state coexists with a long range modulated magnetic order in a narrow region above the reentrant temperature T<sub>c</sub><sub>2</sub>.</p><p>The upper critical magnetic field is a very important magnetic superconductivity parameter. Therefore, starting from its discovery as a superconducting material, experiments are carried out to analysis the upper critical magnetic field (H<sub>c</sub><sub>2</sub>) of HoMo<sub>6</sub>Se<sub>8</sub>.</p><p>According to magnetization measurements, on both poly and single crystalline samples of the ferromagnetic superconducting HoMo<sub>6</sub>Se<sub>8</sub>, the upper critical magnetic field is a turning point from the superconducting state to the normal state. The first-order phase transition is the inter changing point of the superconducting state to the normal state observed when the external field H is applied parallel to the magnetically easy axis (a axis of the hexagonal-rhombohedral crystal lattice structure).</p><p>The critical magnetic field in type-I superconductor is the inter changing point of superconducting state into</p><p>normal state. From Maxwell’s Equation, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x5.png" xlink:type="simple"/></inline-formula>, when the magnetic field is frozen, the field is expelled</p><p>from the interior of the superconductors, otherwise superconductivity will be destroyed by a critical magnetic field (H<sub>c</sub>), such that</p><disp-formula id="scirp.58321-formula193"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x6.png"  xlink:type="simple"/></disp-formula><p>Equation (1) yields the expression of thermodynamic critical magnetic field <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x7.png" xlink:type="simple"/></inline-formula> [<xref ref-type="bibr" rid="scirp.58321-ref9">9</xref>] .</p></sec><sec id="s2"><title>2. Mathematical Formulations to Find the Upper Critical Magnetic Field of HoMo<sub>6</sub>Se<sub>8</sub></title><sec id="s2_1"><title>2.1. The Basic Ginzburg-Landau Theory</title><p>Ginzburg-Landau (GL) theory is a mathematical theory used to describe superconductivity. Ginzburg-Landau (GL) theory is used to explain the difference between Type-I and Type-II superconductors and enables the calculation of two critical magnetic fields H<sub>c</sub><sub>1</sub> and H<sub>c</sub><sub>2</sub> [<xref ref-type="bibr" rid="scirp.58321-ref10">10</xref>] . Ginzburg-Landau theory was derived from the BCS microscopic theory by Lev Gorkov, showing that it also appears in some limit of microscopic theory and applying microscopic interpretation of all its parameters.</p><p>The basic postulate of GL is that if ψ is small and varies slowly in space, the free-energy density <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x8.png" xlink:type="simple"/></inline-formula> can be expanded in a series of the form:</p><disp-formula id="scirp.58321-formula194"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x9.png"  xlink:type="simple"/></disp-formula><p>where α and β are phenomenological parameters, (β is positive and the sign of α is temperature dependent), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x10.png" xlink:type="simple"/></inline-formula>is an effective mass, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x11.png" xlink:type="simple"/></inline-formula>is the charge of an electron, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x12.png" xlink:type="simple"/></inline-formula>is the magnetic vector potential and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x13.png" xlink:type="simple"/></inline-formula> is the magnetic field [<xref ref-type="bibr" rid="scirp.58321-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref10">10</xref>] .</p><p>If<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x14.png" xlink:type="simple"/></inline-formula>, Equation (2) reduces to the free energy of the normal state;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x15.png" xlink:type="simple"/></inline-formula>.</p><p>Now, by minimizing the free energy with respect to fluctuations in the order parameter and the vector potential, one arrives at the Ginzburg-Landau Equations given by:</p><disp-formula id="scirp.58321-formula195"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x16.png"  xlink:type="simple"/></disp-formula><p>The current density from the Hamilton’s energy of particles is given by;</p><disp-formula id="scirp.58321-formula196"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x17.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula197"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x18.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula198"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x19.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x20.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.58321-formula199"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x21.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula200"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x22.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x23.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.58321-formula201"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x24.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula202"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x25.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula203"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x26.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x27.png" xlink:type="simple"/></inline-formula> is supercurrent density.</p><p>Equation (3) determines the order parameter ψ based on the applied magnetic field and Equation (5) yields the superconducting current density. The Ginzburg-Landau Equation provides complete information about the superconducting state <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x28.png" xlink:type="simple"/></inline-formula> that gives the spatial distribution of the Cooper pair density taking into account a possible variation in their concentration, where as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x29.png" xlink:type="simple"/></inline-formula> describes the local distribution of the magnetic field in the superconductor.</p><p>In the absence of external magnetic field (at free surface), there will not be superconducting current(current flow) and the Equation for ψ becomes:</p><disp-formula id="scirp.58321-formula204"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x30.png"  xlink:type="simple"/></disp-formula><p>This Equation has a trivial solution ψ = 0 and it corresponds to normal state of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x31.png" xlink:type="simple"/></inline-formula>. Below superconducting transition temperature (T<sub>c</sub>), Equation (6) is expected to have a non-trivial solution (i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x31.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x32.png" xlink:type="simple"/></inline-formula>) and the Equation can be rearranged into:</p><disp-formula id="scirp.58321-formula205"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x33.png"  xlink:type="simple"/></disp-formula><p>If the second part of Equation (3) is positive, then there is a non zero solution for ψ and this can be achieved</p><p>by assuming the temperature dependence of α such that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x34.png" xlink:type="simple"/></inline-formula> with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x35.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x36.png" xlink:type="simple"/></inline-formula>. For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x37.png" xlink:type="simple"/></inline-formula>, the expression <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x38.png" xlink:type="simple"/></inline-formula> is positive and the second part of Equation (3) is negative and only ψ = 0</p><p>solves the Ginzburg-Landau Equation. For<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x39.png" xlink:type="simple"/></inline-formula>, the second part of Equation (3) is positive and there is a non-trivial solution for ψ. Thus Equation (7) can be expressed as:</p><disp-formula id="scirp.58321-formula206"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x40.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula207"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x41.png"  xlink:type="simple"/></disp-formula><p>Equation (8) yields Ginzburg Landau order parameter [<xref ref-type="bibr" rid="scirp.58321-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref11">11</xref>] .</p></sec><sec id="s2_2"><title>2.2. Calculation of Ginzburg-Landau Coherence Length</title><p>The Ginzbrug-Landau coherence length (ξ<sub>GL</sub>) is a measure of the distance in the superconducting electron concentration that can not change drastically in a spatially-varying magnetic field. The Ginzbrug-Landau coherence length (ξ<sub>GL</sub>) is a temperature-dependent as well as a material dependent quantity. In the case of absence of the magnetic vector potential, Equation (3) reduces to:</p><disp-formula id="scirp.58321-formula208"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x42.png"  xlink:type="simple"/></disp-formula><p>Now, let us consider a wave function that varies only in the z-direction with zero applied magnetic field. In this case, the first GL Equation is one dimensional.</p><p>i.e,</p><disp-formula id="scirp.58321-formula209"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x43.png"  xlink:type="simple"/></disp-formula><p>Assuming ψ is real and neglecting the term <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x44.png" xlink:type="simple"/></inline-formula> in comparison with α, Equation (10), becomes:</p><disp-formula id="scirp.58321-formula210"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x45.png"  xlink:type="simple"/></disp-formula><p>For the plane wave function, the solution of Equation (11) is in the form of,</p><disp-formula id="scirp.58321-formula211"><label>(12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x46.png"  xlink:type="simple"/></disp-formula><p>Substituting the value of plane wave function into Equation (11) (in terms of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x47.png" xlink:type="simple"/></inline-formula>), we get,</p><disp-formula id="scirp.58321-formula212"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x48.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula213"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x49.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula214"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x50.png"  xlink:type="simple"/></disp-formula><p>This implies that,</p><disp-formula id="scirp.58321-formula215"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x51.png"  xlink:type="simple"/></disp-formula><p>Solving for ξ<sub>GL</sub> at superconducting state that means, where α is negative yields,</p><disp-formula id="scirp.58321-formula216"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x52.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x53.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x54.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x55.png" xlink:type="simple"/></inline-formula></p><p>Equation (14) yields the GL coherence length [<xref ref-type="bibr" rid="scirp.58321-ref2">2</xref>] . Since α depends on temperature as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x56.png" xlink:type="simple"/></inline-formula>, then we can conclude that coherence length is temperature dependent.</p><p>Now let us consider the cases:</p><p>Case (I), For superconducting state (T &lt; T<sub>c</sub>),</p><disp-formula id="scirp.58321-formula217"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x57.png"  xlink:type="simple"/></disp-formula><p>and</p><p>Case (II), For normal state (T &gt; T<sub>c</sub>),</p><disp-formula id="scirp.58321-formula218"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x58.png"  xlink:type="simple"/></disp-formula><p>Case (III), at T = T<sub>c</sub>, the GL theory is not valid</p><p>Where the length ξ<sub>GL</sub><sub>(0)</sub> is known as the zero temperature GL coherence length.</p></sec><sec id="s2_3"><title>2.3. Calculation of Ginzburg-Landau Penetration Depth</title><p>The surface current flows in a very thin layer of thickness (λ<sub>GL</sub>) which is called the Ginzburg-Landau penetration depth [<xref ref-type="bibr" rid="scirp.58321-ref2">2</xref>] . The temperature and magnetic field dependence of the penetration depth appear quite naturally in Ginzburg-Landau (GL) theory. Like the London model, the GL model is independent of the underlying mechanism for superconductivity. Ginzburg-Landau theory is strictly valid only in superconducting phase boundary and is thus not generally applicable at low temperatures [<xref ref-type="bibr" rid="scirp.58321-ref2">2</xref>] . In the Ginzburg-Landau theory, a complex order parameter(ψ) is a function of temperature, magnetic field and the spatial coordinates [<xref ref-type="bibr" rid="scirp.58321-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref10">10</xref>] . The total free energy per unit volume of the superconducting state in the presence of a magnetic field is minimizing this expression with respect to the first GL Equation and with respect to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x59.png" xlink:type="simple"/></inline-formula> the current density(GL-II) Equation;</p><disp-formula id="scirp.58321-formula219"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x60.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x61.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x61.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x62.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.58321-formula220"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x63.png"  xlink:type="simple"/></disp-formula><p>Using Equation (17), we get the expression for current density, as follows</p><disp-formula id="scirp.58321-formula221"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x64.png"  xlink:type="simple"/></disp-formula><p>since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x65.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.58321-formula222"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x66.png"  xlink:type="simple"/></disp-formula><p>Neglecting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x67.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x67.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x68.png" xlink:type="simple"/></inline-formula> Equation (20), becomes;</p><disp-formula id="scirp.58321-formula223"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x69.png"  xlink:type="simple"/></disp-formula><p>Using Maxwell’s Equation:</p><disp-formula id="scirp.58321-formula224"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x70.png"  xlink:type="simple"/></disp-formula><p>Taking the curl on both sides of Equation (22), we get</p><disp-formula id="scirp.58321-formula225"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x71.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula226"><label>(24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x72.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x73.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x74.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x73.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x74.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x75.png" xlink:type="simple"/></inline-formula></p><p>From Equation (22) and Equation (24), we get</p><disp-formula id="scirp.58321-formula227"><label>(25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x76.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula228"><label>(26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x77.png"  xlink:type="simple"/></disp-formula><p>Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x78.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x78.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x79.png" xlink:type="simple"/></inline-formula>, we get</p><disp-formula id="scirp.58321-formula229"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x80.png"  xlink:type="simple"/></disp-formula><p>Therefore,</p><disp-formula id="scirp.58321-formula230"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x81.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula231"><label>(29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x82.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x83.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x83.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x84.png" xlink:type="simple"/></inline-formula>.</p><p>Therefore,</p><disp-formula id="scirp.58321-formula232"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x85.png"  xlink:type="simple"/></disp-formula><p>For</p><disp-formula id="scirp.58321-formula233"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x86.png"  xlink:type="simple"/></disp-formula><p>from Equation (30) [<xref ref-type="bibr" rid="scirp.58321-ref9">9</xref>] it follows that, the Ginzburg-Landua penetration depth (λ<sub>GL</sub><sub>(T)</sub>) varies as a function of temperature as:</p><disp-formula id="scirp.58321-formula234"><label>(32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x87.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula235"><label>(33)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x88.png"  xlink:type="simple"/></disp-formula><p>where λ<sub>L</sub><sub>(0)</sub> is the London penetration at absolute zero temperature [<xref ref-type="bibr" rid="scirp.58321-ref9">9</xref>] .</p></sec><sec id="s2_4"><title>2.4. Calculation of the Upper Critical Magnetic Field Using Ginzburg-Landau Theory</title><p>The upper critical magnetic field (UCMF) is the magnetic field which completely suppresses superconductivity in type-II superconductors. More properly, the UCMF is a function of temperature (and pressure) and if not specified absolute zero and standard pressure are implied. Supercondcting region nucleates spontaneously within a normal conductor when the applied magnetic field is decreased below a value denoted by H<sub>c</sub><sub>2</sub> [<xref ref-type="bibr" rid="scirp.58321-ref8">8</xref>] . At the onset of superconductivity, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x89.png" xlink:type="simple"/></inline-formula>is small and we linearize the GL Equations as follows;</p><disp-formula id="scirp.58321-formula236"><label>(34)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x90.png"  xlink:type="simple"/></disp-formula><p>Since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x91.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x92.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x93.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x91.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x92.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x94.png" xlink:type="simple"/></inline-formula>.</p><p>The upper critical magnetic field (H<sub>c</sub><sub>2</sub>) can be calculated by linearizing Equation (34) and substituting the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x95.png" xlink:type="simple"/></inline-formula> as:</p><disp-formula id="scirp.58321-formula237"><label>(35)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x96.png"  xlink:type="simple"/></disp-formula><p>The magnetic field in a superconducting region at the onset of superconductivity is just the applied field, so that <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x97.png" xlink:type="simple"/></inline-formula> and Equation (35) becomes</p><disp-formula id="scirp.58321-formula238"><label>(36)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x98.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x99.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x99.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x100.png" xlink:type="simple"/></inline-formula> where the eigne value of mo-</p><p>mentum crystal is<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x101.png" xlink:type="simple"/></inline-formula>.</p><p>Therefore,</p><disp-formula id="scirp.58321-formula239"><label>(37)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x102.png"  xlink:type="simple"/></disp-formula><p>Since the expression of the Hamiltonian’s energy given in Equation (37) does not depend on coordinates (y and z) the corresponding momentum components (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x103.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x103.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x104.png" xlink:type="simple"/></inline-formula>) are conserved.</p><disp-formula id="scirp.58321-formula240"><label>(38)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x105.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula241"><label>(39)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x106.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula242"><label>(40)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x107.png"  xlink:type="simple"/></disp-formula><p>The largest value of the magnetic field (B) for which the solution of Equation (40) of the lowest eigenvalue is given by</p><disp-formula id="scirp.58321-formula243"><label>(41)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x108.png"  xlink:type="simple"/></disp-formula><p>Let us take the smallest eigenvalues n = 0 and K<sub>z</sub> = 0 corresponding to the highest field in which superconductivity can nucleate in the interior of a bulk sample which occurs with the upper critical magnetic field in the coefficients change of sign. From Equation (41), we have;</p><disp-formula id="scirp.58321-formula244"><label>(42)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x109.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x110.png" xlink:type="simple"/></inline-formula> is the cyclotron frequency and is given by</p><disp-formula id="scirp.58321-formula245"><label>(43)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x111.png"  xlink:type="simple"/></disp-formula><p>since<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x112.png" xlink:type="simple"/></inline-formula>, solving for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x112.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x113.png" xlink:type="simple"/></inline-formula>, we get:</p><disp-formula id="scirp.58321-formula246"><label>(44)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x114.png"  xlink:type="simple"/></disp-formula><p>From the relation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x115.png" xlink:type="simple"/></inline-formula> that means<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x116.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x117.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x115.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x116.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x117.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x118.png" xlink:type="simple"/></inline-formula>.</p><p>We obtain the expression of the temperature dependent upper critical magnetic field (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x119.png" xlink:type="simple"/></inline-formula>),</p><disp-formula id="scirp.58321-formula247"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x120.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula248"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x121.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula249"><label>(45)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x122.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x123.png" xlink:type="simple"/></inline-formula> or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x124.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x123.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x124.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x125.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.58321-formula250"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x126.png"  xlink:type="simple"/></disp-formula></sec><sec id="s2_5"><title>2.5. Anisotropic Mass Tensor Model</title><p>Now, consider anisotropy in mass, by introducing the effective mass tensor to the kinetic energy term of the GL Equation (3), i.e.</p><disp-formula id="scirp.58321-formula251"><label>(46)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x127.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x128.png" xlink:type="simple"/></inline-formula> is an effective mass tensor which is given by,</p><disp-formula id="scirp.58321-formula252"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x129.png"  xlink:type="simple"/></disp-formula><p>Since the coherence length <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x130.png" xlink:type="simple"/></inline-formula> depends on the effective mass as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x130.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x131.png" xlink:type="simple"/></inline-formula>, the resulting Equation is</p><p>formally identical with the Schr&#246;dinger Equation of a particle with charge<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x132.png" xlink:type="simple"/></inline-formula>, an isotropic mass tensor <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x132.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x133.png" xlink:type="simple"/></inline-formula> in a uniform magnetic field H and the energy levels that have the harmonic oscillator are given by;</p><disp-formula id="scirp.58321-formula253"><label>(47)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x134.png"  xlink:type="simple"/></disp-formula><p>Let us consider Newton’s law of motion under the influence of lorentz force</p><p>i.e.</p><disp-formula id="scirp.58321-formula254"><label>(48)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x135.png"  xlink:type="simple"/></disp-formula><p>where v is the velocity.</p><p>The upper critical magnetic field can be expressed by using cyclotron frequency with the lowest free energy;</p><disp-formula id="scirp.58321-formula255"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x136.png"  xlink:type="simple"/></disp-formula><p>The solution of upper critical magnetic field by applying elliptical orbits traversed with cyclotron frequency is given by,</p><disp-formula id="scirp.58321-formula256"><label>(49)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x137.png"  xlink:type="simple"/></disp-formula><p>The solution of the lowest free energy corresponds to n = 0 and by using Equation (49), we get</p><disp-formula id="scirp.58321-formula257"><graphic  xlink:href="http://html.scirp.org/file/1-4800297x138.png"  xlink:type="simple"/></disp-formula><p>where θ is the angle of the magnetic field that makes with the z-axis</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x139.png" xlink:type="simple"/></inline-formula>.</p><disp-formula id="scirp.58321-formula258"><label>(50)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x140.png"  xlink:type="simple"/></disp-formula><p>From the general expression of coherence length Equation (45) we have,</p><disp-formula id="scirp.58321-formula259"><label>(51)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x141.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58321-formula260"><label>(52)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x142.png"  xlink:type="simple"/></disp-formula><p>Using the expression for the flux quantization, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x143.png" xlink:type="simple"/></inline-formula>and Equation (45), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x143.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x144.png" xlink:type="simple"/></inline-formula>can be expressed as,</p><disp-formula id="scirp.58321-formula261"><label>(53)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x145.png"  xlink:type="simple"/></disp-formula><p>For fields parallel and perpendicular to the symmetry plane we can write Equation (53) as:</p><disp-formula id="scirp.58321-formula262"><label>(54)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x146.png"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.58321-formula263"><label>(55)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/1-4800297x147.png"  xlink:type="simple"/></disp-formula><p>Equations (54) and (55) are the mathematical expressions of the upper critical magnetic field (H<sub>c</sub><sub>2</sub>) for fields parallel and perpendicular to the symmetry axis [<xref ref-type="bibr" rid="scirp.58321-ref4">4</xref>] .</p></sec></sec><sec id="s3"><title>3. Results and Discussion</title><p>From Equation (15), we obtained the graph that shows the relationship between the GL coherence length and temperature (T) as indicated in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>As can be see from <xref ref-type="fig" rid="fig1">Figure 1</xref>, the GL coherence length increases with temperature and diverge as<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x148.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x149.png" xlink:type="simple"/></inline-formula>has the same value with the BCS coherence length i.e. (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x148.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x149.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/1-4800297x150.png" xlink:type="simple"/></inline-formula>) [<xref ref-type="bibr" rid="scirp.58321-ref2">2</xref>] .</p><p>We have already calculated the GL penetration depth in (33), the relationship between the GL penetration depth and temperature(T) is shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>.</p><p>From <xref ref-type="fig" rid="fig2">Figure 2</xref>, we observe that, the increase of the GL penetration depth with temperature (T) and generally, we observe that, the penetration depth rises asymptotically as the temperature approaches T<sub>c</sub>. Thus, the pene- tration of field increase as the temperature approaches to T<sub>c</sub>.</p><p>We finally determined the expression for upper critical magnetic field for superconducting HoMo<sub>6</sub>Se<sub>8</sub> using the GL Equation (45) and by taking experimental data and upper critical magnetic fields for parallel and perpendicular, we plot the upper critical fields at parallel and perpendicular to the symmetry axis as shown in <xref ref-type="fig" rid="fig3">Figure 3</xref> [<xref ref-type="bibr" rid="scirp.58321-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.58321-ref7">7</xref>] .</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> GL coherence length versus temperature (T)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800297x151.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> GL penetration depth versus temperature (T)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800297x152.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Upper critical magnetic field parallel and perpendicular to the symmetry axis versus temperature (T)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/1-4800297x153.png"/></fig><p>From <xref ref-type="fig" rid="fig3">Figure 3</xref>, we can see that, the upper critical magnetic field decreases as temperature increases and reaches to zero at the critical temperature of superconducting HoMo<sub>6</sub>Se<sub>8</sub>, which agrees with the experimental observations [<xref ref-type="bibr" rid="scirp.58321-ref6">6</xref>] . And as can be seen from $, the upper critical magnetic field (H<sub>c</sub><sub>2</sub>) parallel and perpendicular to the symmetry axis of superconducting HoMo<sub>6</sub>Se<sub>8</sub> is inversely proportional to the GL coherence length and fits.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The aim of this research is to determine the upper critical field of superconducting HoMo<sub>6</sub>Se<sub>8</sub> by using Ginzburg-Landau approach. From the calculation, the effect of coherence length, penetration depth and anisotropy in mass tensor on upper critical field are considered in our model. And finally figures are plotted by using MATLAB scripts. From the figures plotted, it can be concluded that the upper critical magnetic field of superconducting HoMo<sub>6</sub>Se<sub>8</sub> is inversely related to temperature which is in agreement with experimental observations [<xref ref-type="bibr" rid="scirp.58321-ref6">6</xref>] .</p></sec><sec id="s5"><title>Cite this paper</title><p>TadesseDesta,PooranSingh,GebregziabherKahsay, (2015) Study of Upper Critical Magnetic Field of Superconducting HoMo<sub>6</sub>Se<sub>8</sub>. World Journal of Condensed Matter Physics,05,105-117. doi: 10.4236/wjcmp.2015.53013</p></sec></body><back><ref-list><title>References</title><ref id="scirp.58321-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Owens, F.J. and Poole, Jr., C.P. (2002) The New Superconductors. Kluwer Academic Publishers, New York.</mixed-citation></ref><ref id="scirp.58321-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Mourachkine, A. 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