<?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">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2016.411208</article-id><article-id pub-id-type="publisher-id">JAMP-72451</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>
 
 
  The Density of Energy States for Nonparabolic Dispersion Law in a Strong Magnetic Field
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>U.</surname><given-names>I. Erkaboev</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Physico-Technical Institute, NGO “Physics-Sun”, Academy of Sciences of Uzbekistan, Tashkent, Uzbekistan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:</corresp></author-notes><pub-date pub-type="epub"><day>10</day><month>11</month><year>2016</year></pub-date><volume>04</volume><issue>11</issue><fpage>2113</fpage><lpage>2116</lpage><history><date date-type="received"><day>October</day>	<month>7,</month>	<year>2016</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>November</month>	<year>27,</year>	</date><date date-type="accepted"><day>November</day>	<month>30,</month>	<year>2016</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>
 
 
   
   For nonparabolic dispersion law is determined by the density of the energy states (Ns) in a quantizing magnetic field. The effect of temperature on the expansion of the Lan-dau levels of electrons semiconductors with the nonquadratic dispersion is studied. The density of states at low temperatures is calculated from data on high-tem- perature Ns. 
  
 
</p></abstract><kwd-group><kwd>Quantizing Magnetic Field</kwd><kwd> The Landau Levels</kwd><kwd> The Model Kane</kwd><kwd>  Nonparabolic Zone</kwd><kwd> The Density of States</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In a study of the energy spectra of electrons in semiconductors and metals exceptional role has played the application of quantizing magnetic fields. In the works of [<xref ref-type="bibr" rid="scirp.72451-ref1">1</xref>] the temperature dependence of the density of states in quantizing magnetic fields were considered as the result of thermal broadening of the Landau levels. In those works studies showed, that the density of states of the continuous spectrum measured at the temperature of liquid nitrogen at low temperatures turns into discrete Landau levels. However, in these works are considered only in the quadratic dispersion law.</p><p>The aim of this work is to determining the temperature dependence of the density of energy states in a quantizing magnetic field for the model Kane and into the effect of temperature of a sample on the results of treatment of experimental data.</p></sec><sec id="s2"><title>2. Determination of the Density of Energy States in a Quantizing Magnetic Field for the Kane Dispersion Law</title><p>In a magnetic field the energy of free electrons with a quadratic dispersion law, and in view of the spinal level splitting energy takes the following form [<xref ref-type="bibr" rid="scirp.72451-ref2">2</xref>]:</p><disp-formula id="scirp.72451-formula153"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x2.png"  xlink:type="simple"/></disp-formula><p>In a magnetic field density of states for a parabolic band is determined by the following expression</p><disp-formula id="scirp.72451-formula154"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x3.png"  xlink:type="simple"/></disp-formula><p>However, if the energy dependence of the wave vector is not described by a quadratic form, such as, for electrons in InSb energy levels of the charge carriers in the magnetic field is not equidistant, since cyclotron mass determined by the expression</p><disp-formula id="scirp.72451-formula155"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x4.png"  xlink:type="simple"/></disp-formula><p>and therefore the cyclotron frequency depends on Е and k<sub>z</sub>.</p><p>Nonparabolicity conduction band in compounds III-IV and II-VI is the result of interaction between the conduction and valence bands three. In magnetic field energy levels for the three bands (apart from the heavy hole band that does not interact with them) are cubic equation [<xref ref-type="bibr" rid="scirp.72451-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.72451-ref4">4</xref>]:</p><disp-formula id="scirp.72451-formula156"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x5.png"  xlink:type="simple"/></disp-formula><p>Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x6.png" xlink:type="simple"/></inline-formula>-energy electrons in the conduction band in view of spin in a quantizing magnetic field, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x7.png" xlink:type="simple"/></inline-formula>-width band-gap, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x8.png" xlink:type="simple"/></inline-formula>-the spin-orbit splitting, P-the matrix element.</p><p>From this condition of the cubic Equation (4) reduces to the square, the solution of which electrons of the conduction band is given by</p><disp-formula id="scirp.72451-formula157"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x9.png"  xlink:type="simple"/></disp-formula><p>Equation (5) is applicable only for narrow-gap semiconductors.</p><p>From Equation (5) we define k<sub>z</sub> without spin:</p><disp-formula id="scirp.72451-formula158"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x10.png"  xlink:type="simple"/></disp-formula><p>We return now to the calculation of the density of states with a nonparabolic dispersion law in a magnetic field. The movement of free electrons along the z axis and is quantized by k<sub>z</sub>. That is,</p><disp-formula id="scirp.72451-formula159"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x11.png"  xlink:type="simple"/></disp-formula><p>According to the expression (6) and (7) the number of states the energy interval from</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x12.png" xlink:type="simple"/></inline-formula>to E:</p><disp-formula id="scirp.72451-formula160"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x13.png"  xlink:type="simple"/></disp-formula><p>Here, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x14.png" xlink:type="simple"/></inline-formula>-the density of the energy states of a Kane dispersion law in a quantizing magnetic field. At <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x15.png" xlink:type="simple"/></inline-formula> expression (10) goes into a parabolic dispersion law (2). In this expression, the temperature-induced broadening of the energy levels is disregarded.</p><p>Thermal broadening of the levels in a magnetic field gives rise to the smoothing of discrete levels. Thermal broadening is to be taken into account using a derivative of the</p><p>energy distribution function of the Fermi-Dirac<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x16.png" xlink:type="simple"/></inline-formula>. At absolute zero of temperature, the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x17.png" xlink:type="simple"/></inline-formula> function transforms into the delta-function of Dirac.</p><p>In order to take into account the temperature dependence of the density of states, we</p><p>expend <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x18.png" xlink:type="simple"/></inline-formula> into series with respect to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x19.png" xlink:type="simple"/></inline-formula> functions (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>We then obtain the density of energy states depending on temperature [<xref ref-type="bibr" rid="scirp.72451-ref1">1</xref>] (<xref ref-type="fig" rid="fig1">Figure 1</xref>):</p><disp-formula id="scirp.72451-formula161"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/72451x20.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Determination of the change in the density of energy states with decreasing temperature in high magnetic fields using the Kane model</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/72451x21.png"/></fig><p>The corresponding expression at <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/72451x22.png" xlink:type="simple"/></inline-formula> transforms into (10).</p></sec><sec id="s3"><title>3. Conclusion</title><p>We developed a new method for determining the density of the energy states in a quantizing magnetic field for the Kane model. For a nonquadratic dispersion law was shown that the density of states in a strong magnetic field at an increased temperature coincides with the density of states in the sample without a magnetic field.</p></sec><sec id="s4"><title>Cite this paper</title><p>Erkaboev, U.I. (2016) The Density of Energy States for Nonparabolic Dispersion Law in a Strong Magnetic Field. Journal of Applied Mathematics and Physics, 4, 2113-2116. http://dx.doi.org/10.4236/jamp.2016.411208</p></sec></body><back><ref-list><title>References</title><ref id="scirp.72451-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Gulyamov, G., Erkaboev, U.I. and Sharibaev. Yu.N. (2014) Semiconductor, 48, 1323-1328.  
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