<?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.2015.53019</article-id><article-id pub-id-type="publisher-id">WJCMP-58603</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>
 
 
  Berry Approach to Intrinsic Anomalous Hall Conductivity in Dilute Magnetic Semiconductors (Ga&lt;sub&gt;1-x&lt;/sub&gt;Mn&lt;sub&gt;x&lt;/sub&gt;As)
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>intayehu</surname><given-names>Mekonnen</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>P.</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-group><aff id="aff1"><addr-line>Department of Physics, Addis Ababa University, Addis Ababa, Ethiopia</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>hailemariamsintayeh@gmail.com(IM)</email>;<email>psinghgbpup@yahoo.com(PS)</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>179</fpage><lpage>186</lpage><history><date date-type="received"><day>22</day>	<month>May</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>2</month>	<year>August</year>	</date><date date-type="accepted"><day>5</day>	<month>August</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  We develop a model Hamiltonian to treat intrinsic anomalous Hall conductivity in dilute magnetic semiconductor (DMS) of type (III, Mn, V) and obtain the Berry potential and Berry curvature which are responsible for intrinsic anomalous Hall conductivity in Ga
  <sub>1-x </sub>Mn
  <sub>x</sub>As DMS. Based on Kubo formalism, we establish the relation between Berry curvature and intrinsic anomalous Hall conductivity. We find that for strong spin-orbit interaction intrinsic anomalous Hall conductivity is quantized which is in agreement with recent experimental observation. In addition, we show that the intrinsic anomalous Hall conductivity (AHC) can be controlled by changing concentration of magnetic impurities as well as exchange field. Since Berry curvature related contribution of anomalous Hall conductivity is believed to be dissipationless, our result is a significant step toward achieving dissipationless electron transport in technologically relevant conditions in emerging of spintronics.
 
</p></abstract><kwd-group><kwd>Berry Potential</kwd><kwd> Berry Curvature</kwd><kwd> Kubo Formalism</kwd><kwd> Anomalous Hall Conductivity</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In 1879, Edwin H. Hall discovered that when a conductor carrying longitudinal current was placed in a vertical magnetic field, the carrier would be pressed against the transverse side of the conductor, which led to an observed transverse voltage. This is called the Hall effect (HE) [<xref ref-type="bibr" rid="scirp.58603-ref1">1</xref>] . After almost one century, the quantum Hall effect was discovered by K. von Klitzing in 1982 in a two-dimensional electron gas (2DEG) at low temperature and strong magnetic field [<xref ref-type="bibr" rid="scirp.58603-ref2">2</xref>] . However, in ferromagnetic metals like Fe, Co, and Ni, and newly discovered DMSs like Ga<sub>1−x</sub>Mn<sub>x</sub>As the Hall effect is anomalous and controlled more by magnetization than by Lorentz forces [<xref ref-type="bibr" rid="scirp.58603-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.58603-ref4">4</xref>] , called the anomalous Hall resistivity and the phenomenon is known as anomalous Hall effect (AHE). This phenomenon attracted both experimental and theoretical interest due to its potential application in emerging science of spintronics [<xref ref-type="bibr" rid="scirp.58603-ref5">5</xref>] . The origin of anomalous Hall effect is believed to be due to spin-orbit (SO) interaction in the presence of spin polarization [<xref ref-type="bibr" rid="scirp.58603-ref6">6</xref>] . On the other hand, DMS of type (III, Mn, V) spin polarization is due to exchange interaction between localized Mn<sup>2+</sup> 3d<sup>5+</sup> spins and holes introduced by substitution of Mn<sup>2+</sup> by Ga<sup>3+</sup> [<xref ref-type="bibr" rid="scirp.58603-ref7">7</xref>] . There are two popular theories to explain anomalous Hall effect seen in ferromagnetic system, named as intrinsic and extrinsic theories,both of these theories involve the SO interaction. The intrinsic theory was first time proposed by Karplus and Luttinger (KL) [<xref ref-type="bibr" rid="scirp.58603-ref8">8</xref>] . It required no impurity (the intrinsic scenario) and extrinsic theory, which was proposed by Smit and Berger; they pointed out the role of the impurity scatterings in the steady state equilibrium and hence in the AHE [<xref ref-type="bibr" rid="scirp.58603-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.58603-ref10">10</xref>] . Among others, the intrinsic theory dominantly plays a rule in dilute magnetic semiconductors of type (III, Mn, VI) and the current understanding on intrinsic theories of anomalous hall conductivity allows us to reformulate it with Berry curvature of quasi-particles [<xref ref-type="bibr" rid="scirp.58603-ref11">11</xref>] -[<xref ref-type="bibr" rid="scirp.58603-ref13">13</xref>] . Accordingly, intrinsic AHE results from curvature of electrons below the Fermi surface, as a consequence of the spin-orbit coupling induced topological properties in Bloch bands [<xref ref-type="bibr" rid="scirp.58603-ref13">13</xref>] . Although this anomalous Hall effect (AHE) has become a standard tool to determine the magnetization of ferromagnet and has been known for more than a century, its mechanism is still under debate. Particular attention has been paid to intrinsic mechanisms based on the Berry phase. According to recent experimental result, the intrinsic version of AHC is quantized [<xref ref-type="bibr" rid="scirp.58603-ref14">14</xref>] .</p><p>In this paper we theoretically study anomalous Hall conductivity. The paper is organized as follows. Firstly we develop model Hamiltonian on basis of above discussion, which obtains analytical expression for Berry potential and Berry curvature; secondly after applying Quantum Kubo formulism the connection between Berry curvature and intrinsic Anomalous Hall conductivity is established.</p></sec><sec id="s2"><title>2. Theoretical Formulation</title><p>We consider two dimensional hole gas (2 DhG) in the presence of Spin-orbit coupling taking the form of the usual Rashba term, exchange field, kinetic energy of itinerant holes in the system.</p><disp-formula id="scirp.58603-formula876"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x5.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.58603-formula877"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x6.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x7.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x8.png" xlink:type="simple"/></inline-formula> are usual kinetic energy of carriers (holes) and band mass of charge carriers (holes) respectively</p><disp-formula id="scirp.58603-formula878"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x9.png"  xlink:type="simple"/></disp-formula><p>Here, h<sub>ex</sub> is exchange field resulting from exchange interaction between localized Mn 3d<sup>5</sup> spins and valence band holes introduced by substitution of Mn<sup>2</sup><sup>+</sup> by Ga<sup>3</sup><sup>+</sup> Our approach is based on mean field treatment and magnetization along perpendicular to k<sub>x</sub> and k<sub>y</sub> plane or along z axis(along the direction of quantization). <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x10.png" xlink:type="simple"/></inline-formula>is spin-orbital interaction term in the form of Rash Hamiltonian which accounts that orbital motion of carriers coupled with its spin is given by</p><disp-formula id="scirp.58603-formula879"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x11.png"  xlink:type="simple"/></disp-formula><p>Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x12.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x13.png" xlink:type="simple"/></inline-formula> are Dirac spin operators along x and y direction respectively and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x14.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x15.png" xlink:type="simple"/></inline-formula> are wave vectors along x and y direction respectively and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x16.png" xlink:type="simple"/></inline-formula> Rashba type of spin-orbit coupling constant. Using Equations (2), (3) and (4) into Equation (1), we rewrite the model Hamiltonian as</p><disp-formula id="scirp.58603-formula880"><label>. (5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x17.png"  xlink:type="simple"/></disp-formula><p>In 2D spin space, application of diagonalization procedures in Equation (5) generates two eigenvalues</p><disp-formula id="scirp.58603-formula881"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x18.png"  xlink:type="simple"/></disp-formula><p>And we have obtained the corresponding normalized eigenvectors for spinor part and its complex conjugate</p><disp-formula id="scirp.58603-formula882"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x19.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58603-formula883"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x20.png"  xlink:type="simple"/></disp-formula><sec id="s2_1"><title>2.1. Berry Potential and Berry Curvature</title><p>Berry potential in momentum space along α, β and γ where α, β and γ designates x, y and z coordinate system respectively were defined in terms of periodic spinor Bloch state and in bands as [<xref ref-type="bibr" rid="scirp.58603-ref15">15</xref>]</p><disp-formula id="scirp.58603-formula884"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x21.png"  xlink:type="simple"/></disp-formula><p>Here <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x22.png" xlink:type="simple"/></inline-formula> Using Equations (7) and (8) into Equation (9) and after some algebra, we obtained the</p><p>Berry potential (connection) along x and y direction in k space as follows</p><disp-formula id="scirp.58603-formula885"><label>. (10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x23.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58603-formula886"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x24.png"  xlink:type="simple"/></disp-formula><p>The Berry curvature along perpendicular to α, β and γ plane is defined using analogical expression for real space magnetic field [<xref ref-type="bibr" rid="scirp.58603-ref15">15</xref>] .</p><disp-formula id="scirp.58603-formula887"><label>. (12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x25.png"  xlink:type="simple"/></disp-formula><p>In two dimensional systems we rewrite as,</p><disp-formula id="scirp.58603-formula888"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x26.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58603-formula889"><label>. (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x27.png"  xlink:type="simple"/></disp-formula><p>Using Equation (9) into Equation (14),</p><disp-formula id="scirp.58603-formula890"><label>(15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x28.png"  xlink:type="simple"/></disp-formula><p>This can be written as compact form after introducing commutation relation and straightforward simplification as</p><disp-formula id="scirp.58603-formula891"><label>(16)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x29.png"  xlink:type="simple"/></disp-formula><p>Since <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x30.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x30.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x31.png" xlink:type="simple"/></inline-formula> commutate each other, we get,</p><disp-formula id="scirp.58603-formula892"><label>(17)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x32.png"  xlink:type="simple"/></disp-formula><p>After introducing identity<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x33.png" xlink:type="simple"/></inline-formula>, Equation (17) becomes,</p><disp-formula id="scirp.58603-formula893"><label>(18)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x34.png"  xlink:type="simple"/></disp-formula><p>After Series of steps we have obtained analytical expression for k-space Berry curvature as</p><disp-formula id="scirp.58603-formula894"><label>(19)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x35.png"  xlink:type="simple"/></disp-formula><p>Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x36.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x37.png" xlink:type="simple"/></inline-formula></p><p>Equation (19) is general equation of K-space Berry curvature in 2 DS having periodic part of eigenfunction (Spinor part) <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x38.png" xlink:type="simple"/></inline-formula>non degenerate case. After applying Equation (19) for 2 DhG in dilute magnetic semiconductor (III, Mn, V) system we rewrite the Berry curvature along z direction in k space as,</p><disp-formula id="scirp.58603-formula895"><label>(20)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x39.png"  xlink:type="simple"/></disp-formula><p>In Equation (20), <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x40.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x41.png" xlink:type="simple"/></inline-formula> are the velocity operators along <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x42.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x40.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x41.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x43.png" xlink:type="simple"/></inline-formula></p><p>which were obtained using our model Hamiltonian in Equation (5)</p><disp-formula id="scirp.58603-formula896"><label>(21)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x44.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.58603-formula897"><label>(22)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x45.png"  xlink:type="simple"/></disp-formula><p>Introducing three dimensional unit vector along x, y and z direction, in two dimensional plane in k space in terms Eigen values as follows</p><disp-formula id="scirp.58603-formula898"><label>(23)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x46.png"  xlink:type="simple"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x47.png" xlink:type="simple"/></inline-formula>, using Equations (21)-(23) into Equation (20) and after straightforward manipulation, we have obtained expression for the Berry curvature in k-space for upper and lower band (&#177;), for system of hole gas subjected to spin-orbital coupling and exchange splitting in dilute magnetic semiconductor of type (III, Mn, V) as shown in Equation (24)</p><disp-formula id="scirp.58603-formula899"><label>. (24)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x48.png"  xlink:type="simple"/></disp-formula><p>The Berry curvature in Equation (24) is responsible for intrinsic Anomalous Hall Conductivity seen in system under consideration.</p><p>The connection between Berry curvature and Anomalous Hall conductivity is obtained using Quantum Kubo formalism in the following section.</p></sec><sec id="s2_2"><title>2.2. Quantum Kubo Formalism and AHC</title><p>The Kubo formula for Hall conductivity for current-current correlated system is given by [<xref ref-type="bibr" rid="scirp.58603-ref16">16</xref>]</p><disp-formula id="scirp.58603-formula900"><label>. (25)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x49.png"  xlink:type="simple"/></disp-formula><p>V is volume of system, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x50.png" xlink:type="simple"/></inline-formula>is basis of eigenvectors of the one particle Hamiltonian <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x51.png" xlink:type="simple"/></inline-formula> of Eigenvalues<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x52.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x53.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x50.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x51.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x52.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x54.png" xlink:type="simple"/></inline-formula> are Fermi Dirac distribution function for band n and m respectively.</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x55.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x56.png" xlink:type="simple"/></inline-formula> are single particle current operators given by <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x57.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x55.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x56.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x57.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x58.png" xlink:type="simple"/></inline-formula>, here α and β are the direction of current density. Considering Equation (26) in static limit (ω = 0) and in clean sample and after applying for system of 2D spin polarized hole gas in DMSs after some manipulation we have obtained the flowing expression for AHC.</p><disp-formula id="scirp.58603-formula901"><label>. (26)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x59.png"  xlink:type="simple"/></disp-formula><p>On view of Equation (20), right side of Equation (26) inside the bracket gives<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x60.png" xlink:type="simple"/></inline-formula>. Hence, we can rewrite Equation (26) as</p><disp-formula id="scirp.58603-formula902"><label>(27)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x61.png"  xlink:type="simple"/></disp-formula><p>Here we have replaced the band indices n and m via &#177; which designates lower occupied (−) and upper empty band (+). In continuous limit it is convenient to replace summation into integration. Therefore, Equation (27) becomes</p><disp-formula id="scirp.58603-formula903"><label>(28)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x62.png"  xlink:type="simple"/></disp-formula><p>Plugging Equation (24) into Equation (28), after some algebra we obtained AH conductivity for lower occupied states at T = 0,</p><disp-formula id="scirp.58603-formula904"><label>. (29)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x63.png"  xlink:type="simple"/></disp-formula><p>In Equation (29) we have considered that at Temperature (T = 0) upper band (+) is empty and has nothing contribution to Hall conductivity. Equation (29) integrated to give</p><disp-formula id="scirp.58603-formula905"><label>(30)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x64.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s3"><title>3. Discussion and Conclusions</title><p>From Equation (8) and Equation (9) we can observe that in absence of spin-orbital coupling (α<sub>R</sub> = 0) Berry potential along x and y direction in k-space goes to zero and in similar manner the Berry curvature in Equation (24) also vanishes as (α<sub>R</sub> = 0) Or/and (h<sub>ex</sub> = 0). Therefore, the origin of Berry potential (connection) as well as Berry curvature in a DMS of type (III, Mn, V) is spin-orbital interaction and exchange field (h<sub>ex</sub>). As seen in <xref ref-type="fig" rid="fig1">Figure 1</xref>, the Berry curvature is peaked at k = 0, and from Equation (27) the curvature is proportional to AHC; hence the maximum anomalous Hall conductivity can be attained for k = 0.</p><p>From Equation (30), if<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x65.png" xlink:type="simple"/></inline-formula>, for strong spin orbit coupling limit, we have approximate value anomalous Hall conductivity as</p><disp-formula id="scirp.58603-formula906"><label>(31)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x66.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> The variation of Berry curvature as function of wave vector k for material constant of intrinsic Rashba spin-orbit coupling constant (α<sub>R</sub> = 10 &#197;eV) and exchange field (h<sub>ex</sub> = 40 meV)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-4800305x67.png"/></fig><p>Equation (31) reveals that intrinsic anomalous Hall conductance is almost quantized which is also supported by recent experimental results [<xref ref-type="bibr" rid="scirp.58603-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.58603-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.58603-ref18">18</xref>] . On the other hand, from Equation (27), the intrinsic anomalous Hall conductance is simply the sum of the Chern numbers (the total Berry flux through the BZ) for all the occupied band.</p><p>From Case II, integrating Equation (29) from <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x68.png" xlink:type="simple"/></inline-formula> to upper empty band<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x68.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x69.png" xlink:type="simple"/></inline-formula>, we obtain anomalous Hall conductivity for lower occupied band is</p><disp-formula id="scirp.58603-formula907"><label>. (32)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-4800305x70.png"  xlink:type="simple"/></disp-formula><p>Our analytical results obtained from Equation (30) are similar to result obtained for intrinsic contribution of anomalous hall conductance by classical approach [<xref ref-type="bibr" rid="scirp.58603-ref19">19</xref>] .</p><p>In <xref ref-type="fig" rid="fig2">Figure 2</xref>, we have plotted the variation anomalous Hall conductivity as function exchange field. As can be seen in <xref ref-type="fig" rid="fig1">Figure 1</xref>, when there is no magnetic interaction (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x71.png" xlink:type="simple"/></inline-formula>), the spin lies in the xy plane but there is no spin polarization along z axis. As a result, intrinsic Hall conductivity is zero. However, As <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x71.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x72.png" xlink:type="simple"/></inline-formula> increases the spin is tilted out of the plane by larger amounts, increasing the phase acquired by the wave function (Berry curvature); as a result anomalous hall conductivity increases a until it reaches a maximum and gradually saturates.</p><p>In <xref ref-type="fig" rid="fig3">Figure 3</xref>, anomalous Hall conductivity increases monotonically as composition of magnetic dopant (x) increases. Hence, it is possible to control intrinsic anomalous Hall conductivity by changing the concentration of magnetic impurities.</p><p>In conclusion we say that, at low temperature, in the presence of strong spin-orbit interaction, the anomalous Hall conductivity is quantized. The interplay between spin-orbit interaction and exchange field introduces Berry curvature which is responsible for intrinsic anomalous Hall effect in dilute magnetic semiconductors (Ga<sub>1</sub><sub>−</sub><sub>x</sub>Mn<sub>x</sub>As). Anomalous Hall conductivity increases monotonically as composition of magnetic dopant (x) increases in mean field theory treatment</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> The Variation of Anomalous Hall conductivity as function of exchange field for material constant of spin-orbit splitting (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x74.png" xlink:type="simple"/></inline-formula>) and exchange field h<sub>ex</sub> 0 to 40 meV</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-4800305x73.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Anomalous Hall conductivity as function of composition of magnetic dopant for material constants of spin-orbit splitting (<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-4800305x76.png" xlink:type="simple"/></inline-formula>) and composition of Mn in GaAs (x = 0 to 0.08)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-4800305x75.png"/></fig></sec><sec id="s4"><title>Acknowledgements</title><p>This work was supported by the school of Graduate studies of Addis Ababa University, Addis Ababa, Ethiopia and Arbaminch University, Arbaminch, Ethiopia.</p></sec><sec id="s5"><title>Cite this paper</title><p>SintayehuMekonnen,P.Singh, (2015) Berry Approach to Intrinsic Anomalous Hall Conductivity in Dilute Magnetic Semiconductors (Ga<sub>1-x</sub>Mn<sub>x</sub>As). 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