<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2016.73033</article-id><article-id pub-id-type="publisher-id">JMP-63882</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>
 
 
  Numerical Verification of Transition’s Energies of Excitons in Quantum Well of ZnO with the Finite Difference Method
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>assirou</surname><given-names>Lô</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>Serigne</surname><given-names>Bira Gueye</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, Sciences and Technics Faculty, University Cheikh Anta Diop UCAD, Dakar, Senegal</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>lobass57@gmail.com(AL)</email>;<email>sbiragy@gmail.com(SBG)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>05</day><month>02</month><year>2016</year></pub-date><volume>07</volume><issue>03</issue><fpage>329</fpage><lpage>334</lpage><history><date date-type="received"><day>22</day>	<month>October</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>23</month>	<year>February</year>	</date><date date-type="accepted"><day>26</day>	<month>February</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>
 
 
  This paper shows that the experimental results of quantum well energy transitions can be found numerically. The cases of several ZnO-ZnMgO wells are considered and their excitonic transition energies were calculated using the finite difference method. In that way, the one-dimensional Schr&#246;dinger equation has been solved by using the BLAS and LAPACK libraries. The numerical results are in good agreement with the experimental ones.
 
</p></abstract><kwd-group><kwd>Quantum Well ZnO-ZnMgO</kwd><kwd> Finite Difference Method</kwd><kwd> Exciton</kwd><kwd> Transition Energy</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>ZnO is a very abundant material in nature, with very interesting physiochemical properties: it is non-toxic and presents high chemical stability. It possesses a direct and large band gap (3.37 eV) at room temperature. Its exciton binding energy of the order of 60 meV, enables the design of laser devices operating at room temperature. Its heterostructures are very interesting for optoelectronic applications.</p><p>In general, the search for the eigenstates of the Hamiltonian is complex. Even analytically soluble case of the hydrogen atom is not strictly in simple form if we neglect the coupling with the electromagnetic field. The Schr&#246;dinger equation, even in one dimension, admits precious few analytic solutions so that in the other cases, it is necessary to use various approximation techniques. Perturbation theory provides analytical expressions in the form of asymptotic expansions around undisturbed exactly solvable problem. Numerical analysis allows the exploration of inaccessible situations by perturbation theory. In fact the continuous Schr&#246;dinger equation is not always the most reasonable choice for realize modeling of semiconductors quantum well, superlatice and nanostructures devices. However, the dependency of the energy state on the wave vector dispersion equation for a bulk semiconductor is very close to a discrete model. And as we know, the realistic physics of the Schr&#246;dinger equation arises from its equivalence to a tightbiding model for crystalline solid [<xref ref-type="bibr" rid="scirp.63882-ref1">1</xref>] , in both the bulk and quantum confinement cases. Furthermore, day-to-day, the analytic solution for tight-binding model of quantum wells has not been presented.</p><p>This study presents a numerical model that allows retrieving transition energies of excitons measured in a ZnO-ZnMgO or other quantum-well. This model is based on the finite difference method [<xref ref-type="bibr" rid="scirp.63882-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.63882-ref3">3</xref>] .</p><p>First, we will present the results of experimental measurements of transition energies of excitons in ZnO quantum well. Then, we propose an one-dimensional model of potential barrier which describes the electronic behavior of these wells. Thus, the corresponding model, which is governed by the Schr&#246;dinger equation in steady state, is solved here with the finite difference method. Finally, we compare the numerical results with the experimental results.</p></sec><sec id="s2"><title>2. Experimental Results and Model</title><p>ZnO-ZnMgO quantum wells have been realized with very high crystallographic and optical quality.</p><sec id="s2_1"><title>2.1. Experimental Details: Growth and Structural Properties</title><p>The samples were grown by plasma-assisted MBE, the metals (Zn and Mg) being evaporated using Knudsen cells and atomic oxygen (O) being activated in a radio-frequency plasma cell [<xref ref-type="bibr" rid="scirp.63882-ref4">4</xref>] . The residual carrier concentration in the vicinity of the ZnO QWs is estimated to be less than 10<sup>16</sup> cm<sup>3</sup>.</p><p>We considered three samples. The first contains only one quantum well of width<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x6.png" xlink:type="simple"/></inline-formula>. The second sample contains two quantum wells of width 2.1 nm and 3.6 nm, respectively. The last and third sample possesses one quantum well of width<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x7.png" xlink:type="simple"/></inline-formula>. A schematic diagram (<xref ref-type="fig" rid="fig1">Figure 1</xref>) and details (<xref ref-type="table" rid="table1">Table 1</xref>) of the quantum structure are presented.</p><p>The Mg content of the barrier layers was in the range of 21% - 22%, varying slightly from sample to sample. The QWs were grown at 480˚C i.e. the investigated samples do not contain any cubic inclusions.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Quantum structure</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/8-7502508x8.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Details of quantum structure</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >QW width (nm)</th><th align="center" valign="middle" >1.6</th><th align="center" valign="middle" >2.1</th><th align="center" valign="middle" >3.6</th><th align="center" valign="middle" >10</th></tr></thead><tr><td align="center" valign="middle" >Mg content (%)</td><td align="center" valign="middle" >20</td><td align="center" valign="middle" >25</td><td align="center" valign="middle" >25</td><td align="center" valign="middle" >17</td></tr><tr><td align="center" valign="middle" >Barrier thickness (nm)</td><td align="center" valign="middle" >200</td><td align="center" valign="middle" >95</td><td align="center" valign="middle" >95</td><td align="center" valign="middle" >130</td></tr><tr><td align="center" valign="middle" >Buffer thickness (nm)</td><td align="center" valign="middle" >100</td><td align="center" valign="middle" >680</td><td align="center" valign="middle" >680</td><td align="center" valign="middle" >510</td></tr></tbody></table></table-wrap></sec><sec id="s2_2"><title>2.2. Structural Characterization and Optical Properties</title><p>X-ray reciprocal space maps of samples grown at 480˚C were performed on the <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x9.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x10.png" xlink:type="simple"/></inline-formula> reflections. While these maps suggest that the ZnMgO barriers are at least partially relaxed for Mg contents larger than 40%, heterostructures having Mg contents in the range of 20% are found to be perfectly lattice matched [<xref ref-type="bibr" rid="scirp.63882-ref4">4</xref>] . The high- quality ZnO-ZnMgO QWs grown on sapphire substrate (Al<sub>2</sub>O<sub>3</sub>(0001)), was demonstrated by means as RHEED, AFM and PL studies. PL spectra of one of these samples recorded at 10 K are displayed in <xref ref-type="fig" rid="fig2">Figure 2</xref>. The high energy peak (3.82 eV) corresponds to the PL emission of the barrier layer with Mg content of 21% - 22%, while the emission at 3.37 eV corresponds to the free exciton recombination from the ZnO template and the other line 3.535 eV is the excitonic emission of the QW of width 1.6 nm.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> concerns the low temperature PL spectra from a 10 nm thick QW (b) embedded in a Zn<sub>0.83</sub>Mg<sub>0.17</sub>O</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> PL spectrum of ZnO QW (L<sub>w</sub> = 1.6 nm)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/8-7502508x11.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> QWs 3.6 nm, 2.1 nm, and 10 nm</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/8-7502508x12.png"/></fig><p>barrier layer grown on R-plane sapphire substrate and from a sample containing two QWs (a) [<xref ref-type="bibr" rid="scirp.63882-ref5">5</xref>] . The excitonic emission from the 10 nm QW emits at 3.39 eV, which is also the energy of the excitonic band gap of A-plane ZnO, while the PL of the Zn<sub>0.83</sub>Mg<sub>0.17</sub>O barrier layer peaks at 3.82 eV.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref>(a) corresponds to the PL lines of a sample containing two QWs of width (3.6 nm) and (2.1 nm), emitting at 3.44 eV and 3.451 eV, respectively. The widths of the QWs were chosen to be sufficiently different so that the corresponding PL emission lines are well separated [<xref ref-type="bibr" rid="scirp.63882-ref5">5</xref>] . So, for the band conduction electrons, a potential barrier of 430 meV and 447 meV is formed. The behavior of the electron in the QW is described by the Schr&#246;dinger equation:</p><disp-formula id="scirp.63882-formula1757"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x13.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x14.png" xlink:type="simple"/></inline-formula> is the electron confinement energy. The correction potential energy due to the difference effective mass between the barrier and the quantum well is neglected. The model we propose able to find the energy confinement of the electron in the QW and then their stationary states. Contrary to other computational approaches [<xref ref-type="bibr" rid="scirp.63882-ref6">6</xref>] , it is more direct. A schematic description of the potential is presented in <xref ref-type="fig" rid="fig4">Figure 4</xref>.</p></sec></sec><sec id="s3"><title>3. Use of the Finite Difference Method</title><p>The Finite Difference method for solving the 1D Time Independent Schr&#246;dinger Equation is presented. This method is a simple and very important tool for physics and engineering where the Schr&#246;dinger equation appears very often in the description of certain phenomena [<xref ref-type="bibr" rid="scirp.63882-ref7">7</xref>] .</p><sec id="s3_1"><title>3.1. Stationary States in 1D Potential</title><p>This is described by the following equation:</p><disp-formula id="scirp.63882-formula1758"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x15.png"  xlink:type="simple"/></disp-formula><p>This is equivalent to</p><disp-formula id="scirp.63882-formula1759"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x16.png"  xlink:type="simple"/></disp-formula><p>This latter can be normalized with</p><disp-formula id="scirp.63882-formula1760"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x17.png"  xlink:type="simple"/></disp-formula><p>Thus we get</p><disp-formula id="scirp.63882-formula1761"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x18.png"  xlink:type="simple"/></disp-formula><p>this equation will be solved with the Finite Difference Method (FDM).</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Potential barrier</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/8-7502508x19.png"/></fig></sec><sec id="s3_2"><title>3.2. Finite Difference Method</title><p>We consider a function specified <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x20.png" xlink:type="simple"/></inline-formula> which satisfies the Schr&#246;dinger equation, in the interval</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x21.png" xlink:type="simple"/></inline-formula>. <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x22.png" xlink:type="simple"/></inline-formula>fulfills the boundary conditions <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x23.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x21.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x22.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x24.png" xlink:type="simple"/></inline-formula>. We con-</p><p>sider an one-dimensional mesh with N + 2 points<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x25.png" xlink:type="simple"/></inline-formula>, where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x25.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x26.png" xlink:type="simple"/></inline-formula> and we define</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x27.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x28.png" xlink:type="simple"/></inline-formula>;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x29.png" xlink:type="simple"/></inline-formula>.</p><p>The FDM is based on the Taylor expansion. So, with the centered difference approximation, the second order derivative of the stationary wave functions can be approximated by the following:</p><disp-formula id="scirp.63882-formula1762"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x30.png"  xlink:type="simple"/></disp-formula><p>Thus, the 1D Time Independent Schr&#246;dinger Equation becomes a set of algebraic equations</p><disp-formula id="scirp.63882-formula1763"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x31.png"  xlink:type="simple"/></disp-formula><p>This is equivalent to following</p><disp-formula id="scirp.63882-formula1764"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x32.png"  xlink:type="simple"/></disp-formula><p>Defining</p><disp-formula id="scirp.63882-formula1765"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x33.png"  xlink:type="simple"/></disp-formula><p>one gets a linear system of N equations, which can be written in a matrix form [<xref ref-type="bibr" rid="scirp.63882-ref3">3</xref>] .</p><disp-formula id="scirp.63882-formula1766"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/8-7502508x34.png"  xlink:type="simple"/></disp-formula><p>To solve this 1D equation means to determine the eigenvalues <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x35.png" xlink:type="simple"/></inline-formula> and thus the eigenvectors<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x35.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/8-7502508x36.png" xlink:type="simple"/></inline-formula>. Equation (10) has been solved with FORTRAN, using the librairies of BLAS and LAPACK for eigenvalue/eigenvactor problems. Particularly, the parameters of our QWs allow us to determine the diagonal elements of the symmetric matrix M. Thus, the eigenvalues of M have been calculated and the energy levels E<sub>n</sub> have been determined. The obtained results are shown in <xref ref-type="table" rid="table2">Table 2</xref>.</p></sec></sec><sec id="s4"><title>4. Verification and Discussions</title><p>A verification of the proposed method is done, considering the results of three samples. It concerns four quantum wells whose widths are 1.6 nm, 2.1 nm, 3.6 nm et 10 nm; respectively.</p><p>The numerical calculation, carried out for all the wells, allowed to recover the experimental results. If we consider the quantum well of width 1.6 nm, the expected emission energies are between 1.45 and 1.65 eV, according to the experimental measurements. The energy levels E1 and E2, calculated with the method of finite difference, correspond to emission energies of 373 meV and 168 meV, respectively. These values obtained are consistent with the experimental results. For the other quantum wells, this agreement between numerical result and experience can be observed. These results are summarized in <xref ref-type="table" rid="table2">Table 2</xref>.</p><p>The proposed numerical method using the finite difference method allows retrieving the experimental values of emission energies of unstrained ZnO-ZnMgO quantum wells where the Stark effect has been neglected.</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Numerical results</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Energy [mev]\QW width</th><th align="center" valign="middle" >L<sub>w</sub> = 1.6 nm V<sub>0</sub> = 447 mev</th><th align="center" valign="middle" >L<sub>w</sub> = 2.1 nm V<sub>0</sub> = 430 mev</th><th align="center" valign="middle" >L<sub>w</sub> = 3.6 nm V<sub>0</sub> = 430 mev</th><th align="center" valign="middle" >L<sub>w</sub> = 10 nm V<sub>0</sub> = 430 mev</th></tr></thead><tr><td align="center" valign="middle" >E1</td><td align="center" valign="middle" >−373</td><td align="center" valign="middle" >−381</td><td align="center" valign="middle" >−410</td><td align="center" valign="middle" >−427</td></tr><tr><td align="center" valign="middle" >E2</td><td align="center" valign="middle" >−168</td><td align="center" valign="middle" >−241</td><td align="center" valign="middle" >−350</td><td align="center" valign="middle" >−417</td></tr><tr><td align="center" valign="middle" >E3</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−42</td><td align="center" valign="middle" >−253</td><td align="center" valign="middle" >−402</td></tr><tr><td align="center" valign="middle" >E4</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−126</td><td align="center" valign="middle" >−381</td></tr><tr><td align="center" valign="middle" >E5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−354</td></tr><tr><td align="center" valign="middle" >E6</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−323</td></tr><tr><td align="center" valign="middle" >E7</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−286</td></tr><tr><td align="center" valign="middle" >E8</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−254</td></tr><tr><td align="center" valign="middle" >E9</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−200</td></tr><tr><td align="center" valign="middle" >E10</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−152</td></tr><tr><td align="center" valign="middle" >E11</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−102</td></tr><tr><td align="center" valign="middle" >E12</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−50</td></tr><tr><td align="center" valign="middle" >E13</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >−1</td></tr></tbody></table></table-wrap></sec><sec id="s5"><title>5. Conclusion</title><p>In summary, we have shown in this paper that the model of one-dimensional quantum wells allows finding excitonic energy levels determined experimentally. By solving the Schr&#246;dinger equation with the finite difference method, we could recover experimental energy levels with high accuracy. A subsequent study could be interested in the case of optically coupled quantum wells, superlatices and atomic latices with sinusoidal potential in plane. This work can be extended to the diffraction of Gaussian wave under Fraunhofer condition.</p></sec><sec id="s6"><title>Cite this paper</title><p>BassirouL&#244;,Serigne BiraGueye, (2016) Numerical Verification of Transition’s Energies of Excitons in Quantum Well of ZnO with the Finite Difference Method. Journal of Modern Physics,07,329-334. doi: 10.4236/jmp.2016.73033</p></sec></body><back><ref-list><title>References</title><ref id="scirp.63882-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Boykin, T.B. (2001) American Journal of Physics, 69, 793-798. http://dx.doi.org/10.1119/1.1344169</mixed-citation></ref><ref id="scirp.63882-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Boykin, T.B. and Klimeck, G. (2004) The Discretized Schrodinger Equation and Simple Models for Semiconductor Quantum Wells.</mixed-citation></ref><ref id="scirp.63882-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">LeVeque, R.J. (2007) Finite Difference Method for Ordinary and Partial Differential Equations, Steady State and Time Dependent Problems. 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