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<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xml:lang="en" article-type="review-article">
  <front>
    <journal-meta>
      <journal-id journal-id-type="publisher-id">symmetry</journal-id>
      <journal-title>Symmetry</journal-title>
      <abbrev-journal-title abbrev-type="publisher">Symmetry</abbrev-journal-title>
      <abbrev-journal-title abbrev-type="pubmed">symmetry</abbrev-journal-title>
      <issn pub-type="epub">2073-8994</issn>
      <publisher>
        <publisher-name>MDPI</publisher-name>
      </publisher>	
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.3390/sym4030452</article-id>
      <article-id pub-id-type="publisher-id">symmetry-04-00452</article-id>
      <article-categories>
        <subj-group>
          <subject>Review</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title>Supersymmetric Quantum Mechanics and Solvable Models</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <name>
            <surname>Bougie</surname>
            <given-names>Jonathan</given-names>
          </name>
          <xref rid="af1-symmetry-04-00452" ref-type="aff">1</xref>
          <xref rid="c1-symmetry-04-00452" ref-type="corresp">*</xref>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Gangopadhyaya</surname>
            <given-names>Asim</given-names>
          </name>
          <xref rid="af1-symmetry-04-00452" ref-type="aff">1</xref>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Mallow</surname>
            <given-names>Jeffry</given-names>
          </name>
          <xref rid="af1-symmetry-04-00452" ref-type="aff">1</xref>
        </contrib>
        <contrib contrib-type="author">
          <name>
            <surname>Rasinariu</surname>
            <given-names>Constantin</given-names>
          </name>
          <xref rid="af2-symmetry-04-00452" ref-type="aff">2</xref>
        </contrib>
      </contrib-group>
      <aff id="af1-symmetry-04-00452"><label>1 </label>Department of Physics, Loyola University Chicago, 1032 W. Sheridan Rd., Chicago, IL 60660, USA; Email: <email>agangop@gmail.com</email> (A.G.); <email>jvmallow@gmail.com</email> (J.M.)</aff>
      <aff id="af2-symmetry-04-00452"><label>2 </label>Department of Science and Mathematics, Columbia College Chicago, 600 S. Michigan Ave., Chicago, IL 60605, USA; Email: <email>crasinariu@colum.edu</email></aff>
      <author-notes>
        <corresp id="c1-symmetry-04-00452"><label>*</label> Author to whom correspondence should be addressed; Email: <email>jbougie@luc.edu</email>; Tel.: +1-773-508-3543; Fax: +1-773-508-3534.</corresp>
      </author-notes>
      <pub-date pub-type="epub">
        <day>14</day>
        <month>08</month>
        <year>2012</year>
      </pub-date>
      <pub-date pub-type="collection"><month>09</month>
        <year>2012</year>
      </pub-date>
      <volume>4</volume>
      <issue>3</issue>
      <fpage>452</fpage>
      <lpage>473</lpage>
      <history>
        <date date-type="received">
          <day>29</day>
          <month>06</month>
          <year>2012</year>
        </date>
        <date date-type="rev-recd">
          <day>20</day>
          <month>07</month>
          <year>2012</year>
        </date>
        <date date-type="accepted">
          <day>31</day>
          <month>07</month>
          <year>2012</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>© 2012 by the authors; licensee MDPI, Basel, Switzerland.</copyright-statement>
        <copyright-year>2012</copyright-year>
        <license xmlns:xlink="http://www.w3.org/1999/xlink" license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/3.0/">
          <p>This article is an open-access article distributed under the terms and conditions of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/3.0/).</p>
        </license>
      </permissions>
      <abstract>
        <p>We review solvable models within the framework of supersymmetric quantum mechanics (SUSYQM). In SUSYQM, the shape invariance condition insures solvability of quantum mechanical problems. We review shape invariance and its connection to a consequent potential algebra. The additive shape invariance condition is specified by a difference-differential equation; we show that this equation is equivalent to an infinite set of partial differential equations. Solving these equations, we show that the known list of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i001.tif"/>-independent superpotentials is complete. We then describe how these equations could be extended to include superpotentials that do depend on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i001.tif"/>.</p>
      </abstract>
      <kwd-group>
        <kwd>supersymmetry</kwd>
        <kwd>quantum mechanics</kwd>
        <kwd>shape invariance</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec>
      <title/>
      <p><bold>Classification:</bold> PACS 03.65.-w, 47.10.-g, 11.30.Pb</p>
    </sec>
    <sec sec-type="intro">
      <title>1. Introduction</title>
      <p>Supersymmetric quantum mechanics (SUSYQM) is a generalization of the factorization method commonly used for the harmonic oscillator. The factorization technique begun by Darboux [<xref ref-type="bibr" rid="B1-symmetry-04-00452">1</xref>] about one hundred years ago, and used by Schrödinger [<xref ref-type="bibr" rid="B2-symmetry-04-00452">2</xref>,<xref ref-type="bibr" rid="B3-symmetry-04-00452">3</xref>,<xref ref-type="bibr" rid="B4-symmetry-04-00452">4</xref>] in the 1940’s and Infeld and Hull in the 1950’s [<xref ref-type="bibr" rid="B5-symmetry-04-00452">5</xref>], could be considered a precursor of SUSYQM.</p>
      <p>The current form of SUSYQM appeared in 1981 [<xref ref-type="bibr" rid="B6-symmetry-04-00452">6</xref>] as a model of dynamical symmetry breaking. It was developed further by the authors of [<xref ref-type="bibr" rid="B8-symmetry-04-00452">8</xref>,<xref ref-type="bibr" rid="B7-symmetry-04-00452">7</xref>] among others. This simplified model turned out to have important applications in quantum mechanics.</p>
      <p>In the next section, we will describe the general formalism of SUSYQM and in <xref ref-type="sec" rid="sec3-symmetry-04-00452">Section 3</xref> we introduce the shape invariance condition that makes a potential solvable. <xref ref-type="sec" rid="sec4-symmetry-04-00452">Section 4</xref> is dedicated to a description of potential algebra and its connection to shape invariance. In <xref ref-type="sec" rid="sec5-symmetry-04-00452">Section 5</xref> we will describe a method for determining solutions of the translational shape invariance condition. We will then conclude with the analysis of recently discovered shape invariant potentials that are inherently functions of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>.</p>
    </sec>
    <sec>
      <title>2. Supersymmetric Quantum Mechanics</title>
      <p>Throughout this paper, we use units such that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i003.tif"/>. For the harmonic oscillator, the Hamiltonian [<xref ref-type="bibr" rid="B9-symmetry-04-00452">9</xref>] <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i004.tif"/> is factorized into <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i005.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i006.tif"/>. Similarly, in the SUSYQM formalism [<xref ref-type="bibr" rid="B10-symmetry-04-00452">10</xref>,<xref ref-type="bibr" rid="B11-symmetry-04-00452">11</xref>] a general Hamiltonian <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i007.tif"/> is written as a product of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i008.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i009.tif"/>, where the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i010.tif"/> is known as the superpotential. The product <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i011.tif"/> is then given by </p>
      <p><disp-formula id="symmetry-04-00452-i012"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i012.tif"/><label>(1)</label></disp-formula></p>
      <p>Thus, the product <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i011.tif"/> indeed reproduces the Hamiltonian <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/> above, provided the potential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i014.tif"/> is related to the superpotential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i010.tif"/> by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i015.tif"/>. The product <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i016.tif"/> produces another Hamiltonian <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i017.tif"/> with <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i018.tif"/>. To see the underlying supersymmetry of this formalism, let us construct a generator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i019.tif"/> and its adjont <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i020.tif"/> by: </p>
      <p><disp-formula id="symmetry-04-00452-i021"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i021.tif"/><label>(2)</label></disp-formula></p>
      <p>Operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i019.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i020.tif"/> generate the following supersymmetry algebra: </p>
      <p><disp-formula id="symmetry-04-00452-i022"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i022.tif"/><label>(3)</label></disp-formula></p>
      <p>The groundstate energy of this Hamiltonian is then given by </p>
      <p><disp-formula id="symmetry-04-00452-i023"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i023.tif"/><label>(4)</label></disp-formula></p>
      <p>Thus, the non-vanishing of the groundstate energy implies that either <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i024.tif"/> or <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i025.tif"/>, and hence signals the spontaneous breaking of the supersymmetry. We therefore require that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i026.tif"/> to preserve unbroken supersymmetry.</p>
      <p>The Hamiltonians <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i027.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/> are intertwined; <italic>i.e.</italic>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i028.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i029.tif"/>. This leads to the following relationships among their eigenvalues and eigenfunctions [<xref ref-type="bibr" rid="B12-symmetry-04-00452">12</xref>] </p>
      <p><disp-formula id="symmetry-04-00452-i030"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i030.tif"/><label>(5)</label></disp-formula></p>
      <p>Since <italic>H<sub>±</sub></italic> are products of the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i031.tif"/> and its adjoint <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i032.tif"/>, their eigenvalues are either zero or positive [<xref ref-type="bibr" rid="B13-symmetry-04-00452">13</xref>]. The ground state eigenvalue of one of these Hamiltonians must be zero in order to have unbroken supersymmetry. Without loss of generality, we choose that Hamiltonian to be <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/>. Thus, we have </p>
      <p><disp-formula id="symmetry-04-00452-i033"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i033.tif"/><label>(6)</label></disp-formula></p>
      <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i034.tif"/> is an arbitrary point in the domain and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i035.tif"/> is the normalization constant that depends on the choice of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i034.tif"/>. Thus, if <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i036.tif"/> is a normalizable groundstate, we have a system with unbroken supersymmetry. Its groundstate <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i037.tif"/> is zero and the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i031.tif"/> annihilates the corresponding eigenstate <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i036.tif"/>. For all higher states of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/>, as indicated in Equation (5), there is an one-to-one correspondence with the states of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i027.tif"/>. </p>
      <sec>
        <title>2.1. Example</title>
        <p>Consider a system described by the superpotential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i038.tif"/>, defined over the domain <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i039.tif"/>. Corresponding partner potentials are given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i040.tif"/>. This is a rather complicated potential, and rarely analyzed in quantum mechanics courses. However, for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i041.tif"/>, the potential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i042.tif"/> reduces to the infinite square well, with the bottom of the potential at <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i043.tif"/> and zero groundstate energy. We know that the corresponding eigenstates are given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i044.tif"/> and eigenvalues <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i045.tif"/>. Thus, using the familiarity with the relatively simpler potential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i046.tif"/>, we are able to derive all of the eigenvalues and eigenfunctions of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i047.tif"/>. Then the inter-relations expressed through Equation (5) enable us to determine eigenvalues and eigenfunctions of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i048.tif"/>.</p>
        <p>Although we assume that our Hamiltonians are hermitian, hermiticity is not necessary to generate real eigenvalues. Replacing the sufficient but not necessary condition of hermiticity with the weaker condition of PT symmetry, has led to the discovery of new potentials with real energy eigenvalues [<xref ref-type="bibr" rid="B14-symmetry-04-00452">14</xref>,<xref ref-type="bibr" rid="B15-symmetry-04-00452">15</xref>,<xref ref-type="bibr" rid="B16-symmetry-04-00452">16</xref>]. Considerable work has been done on the study of SI potentials with PT symmetry. In reference [<xref ref-type="bibr" rid="B17-symmetry-04-00452">17</xref>], the author examined the shape invariant hyperbolic Rosen-Morse potential as a case of exact solvability with PT invariance. In reference [<xref ref-type="bibr" rid="B18-symmetry-04-00452">18</xref>], the Scarf II potential was shown as an example of spontaneous PT-symmetry-breaking. The case of a square well with discrete PT symmetry but with intervals of non-hermiticity was shown in reference [<xref ref-type="bibr" rid="B19-symmetry-04-00452">19</xref>] to produce real eigenvalues. Authors of [<xref ref-type="bibr" rid="B20-symmetry-04-00452">20</xref>] constructed the spectrum of a square well of imaginary strength, to obtain the hierarchy of SI potentials, while authors of [<xref ref-type="bibr" rid="B21-symmetry-04-00452">21</xref>] constructed a set of solvable rational potentials, and related the PT symmetry condition to the condition that they be free of singularities. However, in this paper we limit ourselves to the case of hermitian Hamiltonians, <italic>i.e.</italic>, real <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i010.tif"/>.</p>
        <p>The remainder of this manuscript is devoted to the study of the shape invariance condition and its solutions.</p>
      </sec>
    </sec>
    <sec id="sec3-symmetry-04-00452">
      <title>3. Shape Invariance in Supersymmetric Quantum Mechanics</title>
      <p>If the superpotential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i049.tif"/> of a system obeys the condition </p>
      <p><disp-formula id="symmetry-04-00452-i050"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i050.tif"/><label>(7)</label></disp-formula></p>
      <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i051.tif"/>, the system is called shape invariant [<xref ref-type="bibr" rid="B5-symmetry-04-00452">5</xref>,<xref ref-type="bibr" rid="B22-symmetry-04-00452">22</xref>,<xref ref-type="bibr" rid="B23-symmetry-04-00452">23</xref>,<xref ref-type="bibr" rid="B24-symmetry-04-00452">24</xref>]. Various forms of the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i052.tif"/> define classes of shape invariance. The most commonly discussed classes are: </p>
      <p><disp-formula id="symmetry-04-00452-i053"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i053.tif"/><label/></disp-formula></p>
      <p>From Equation (7) it follows that for a shape invariant system, the partner potentials <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i054.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i055.tif"/> differ only by values of parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i056.tif"/> and additive constants <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i057.tif"/>. In particular, </p>
      <p><disp-formula id="symmetry-04-00452-i058"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i058.tif"/><label>(8)</label></disp-formula></p>
      <p>In terms of operators <italic>A<sub>±</sub></italic>, the shape invariance condition becomes </p>
      <p><disp-formula id="symmetry-04-00452-i059"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i059.tif"/><label>(9)</label></disp-formula></p>
      <p>As we will see in <xref ref-type="sec" rid="sec4-symmetry-04-00452">Section 4</xref>, Equation (9) implies that for every shape invariant system, there is always an underlying potential algebra [<xref ref-type="bibr" rid="B28-symmetry-04-00452">28</xref>,<xref ref-type="bibr" rid="B30-symmetry-04-00452">30</xref>,<xref ref-type="bibr" rid="B29-symmetry-04-00452">29</xref>,<xref ref-type="bibr" rid="B32-symmetry-04-00452">32</xref>,<xref ref-type="bibr" rid="B31-symmetry-04-00452">31</xref>] that guarantees its solvability. In the rest of this section, we will show how shape invariance enables us to find the eigenvalues and eigenfunctions of the system.</p>
      <sec>
        <title>3.1. Determination of Eigenvalues</title>
        <p>From Equation (9), we see that Hamiltonians <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i060.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i061.tif"/> differ only by the constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i062.tif"/>. We already know that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i063.tif"/>. Let us determine the first excited state of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/>; <italic>i.e.</italic>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i064.tif"/>. Hence, using <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i065.tif"/>[<xref ref-type="bibr" rid="B33-symmetry-04-00452">33</xref>], we find that the energy <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i064.tif"/> of the first excited state of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i066.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i067.tif"/> of the groundstate of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i060.tif"/> both are given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i062.tif"/>. Similarly, to determine <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i068.tif"/>, we use the isospectrality condition (5) to relate it to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i069.tif"/>. But by the shape invariance condition (9), <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i069.tif"/>= <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i070.tif"/>. Following the method used for determining <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i064.tif"/>, we find <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i071.tif"/>, and hence, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i072.tif"/>. Extending this argument to higher excited states of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i066.tif"/>, we get</p>
        <p><disp-formula id="symmetry-04-00452-i073"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i073.tif"/><label>(10)</label></disp-formula></p>
      </sec>
      <sec>
        <title>3.2 Determination of Eigenfunctions</title>
        <p>Again from Equation (9), we see that since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i060.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i061.tif"/> only differ by the constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i062.tif"/>, they must have common eigenfunctions. Hence, from Equation (6), we have <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i074.tif"/>. Then the isospectrality condition (5), requires <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i075.tif"/>. Iterating this procedure, we obtain </p>
        <p><disp-formula id="symmetry-04-00452-i076"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i076.tif"/><label>(11)</label></disp-formula></p>
        <p>Thus, for a system with a given shape invariant superpotential, the eigenvalues and eigenfunctions can be determined analytically. This result makes it very important to find all such potentials. In the past, researchers had found a list of additive shape invariant potentials [<xref ref-type="bibr" rid="B10-symmetry-04-00452">10</xref>,<xref ref-type="bibr" rid="B11-symmetry-04-00452">11</xref>], mostly by trial and error [<xref ref-type="bibr" rid="B34-symmetry-04-00452">34</xref>,<xref ref-type="bibr" rid="B35-symmetry-04-00452">35</xref>]. In <xref ref-type="sec" rid="sec5-symmetry-04-00452">Section 5</xref>, we will discuss how to find solutions of Equation (9) for the additive case. Before that, however, in the next section we will show why the shape invariance condition leads to solvability.</p>
      </sec>
    </sec>
    <sec id="sec4-symmetry-04-00452">
      <title>4. Shape Invariance and Potential Algebra</title>
      <p>We will now show that the symmetry behind the shape invariance is essential in building the algebraic structures known as <italic>potential algebras</italic>. As we will show below, a potential algebra is in general a deformation of a three-dimensional Lie algebra, whose representations yield the spectrum of the corresponding shape invariant system.</p>
      <sec>
        <title>4.1. Building the Algebra</title>
        <p>The starting point of our construct is the shape invariance condition given by Equation (9), which we rewrite as </p>
        <p><disp-formula id="symmetry-04-00452-i077"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i077.tif"/><label>(12)</label></disp-formula></p>
        <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i078.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i052.tif"/> is a function that models the change of parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i079.tif"/>. For example, if the change of parameter is a translation, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i080.tif"/>.</p>
        <p>The left hand side of Equation (12) resembles a commutation relation. This suggests that we use <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i031.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i032.tif"/> to build the generators of the potential algebra. To transform the above shape invariance condition into an exact commutator, we replace operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i081.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i082.tif"/> by</p>
        <p><disp-formula id="symmetry-04-00452-i083"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i083.tif"/><label>(13)</label></disp-formula></p>
        <p>where  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i084.tif"/> is a constant parameter, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i085.tif"/> is an auxiliary variable, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i086.tif"/>. The function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/> will be appropriately chosen to emulate the relationship between parameters <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i088.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i089.tif"/>. Thus, to generate <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/>, we multiplied the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i081.tif"/> from right by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i091.tif"/> and replaced the parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i088.tif"/> by the differential operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i092.tif"/>. If we now compute the commutator between operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i093.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/>, we find [<xref ref-type="bibr" rid="B36-symmetry-04-00452">36</xref>]</p>
        <p><disp-formula id="symmetry-04-00452-i094"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i094.tif"/><label>(14)</label></disp-formula></p>
        <p>Observe now that the right hand side of Equation (14) matches the left hand side of Equation (12) provided that we make the following mappings</p>
        <p><disp-formula id="symmetry-04-00452-i095"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i095.tif"/><label>(15)</label></disp-formula></p>
        <p>Since we know that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i079.tif"/>, these mappings require that the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i096.tif"/> satisfy</p>
        <p><disp-formula id="symmetry-04-00452-i097"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i097.tif"/><label>(16)</label></disp-formula></p>
        <p>Let us look at some examples to illustrate this procedure. </p>
        <p>• Translation: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i080.tif"/></p>
        <p>If the change of parameters is a translation, then the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/> that models it is the identity function</p>
        <p><disp-formula id="symmetry-04-00452-i098"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i098.tif"/><label>(17)</label></disp-formula></p>
        <p>We have <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i099.tif"/>, which gives the desired change of parameters.</p>
        <p>• Scaling: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i100.tif"/></p>
        <p>For shape invariant potentials characterized by a scaling change of parameters, the corresponding function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/> is the exponential</p>
        <p><disp-formula id="symmetry-04-00452-i101"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i101.tif"/><label>(18)</label></disp-formula></p>
        <p>Indeed <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i102.tif"/> where we denoted <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i103.tif"/>.</p>
        <p>• Cyclic: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i104.tif"/></p>
        <p>Cyclic potentials form a series of shape invariant potentials that repeats after a cycle of  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i105.tif"/> iterations. These potentials appear also in connection with the dressing chain formalism [<xref ref-type="bibr" rid="B37-symmetry-04-00452">37</xref>]. To satisfy the cyclic parameter change, the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i052.tif"/> should obey <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i106.tif"/>. The projective map <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i107.tif"/> with specific constraints [<xref ref-type="bibr" rid="B38-symmetry-04-00452">38</xref>] on the parameters <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i108.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i109.tif"/> satisfies such a condition [<xref ref-type="bibr" rid="B27-symmetry-04-00452">27</xref>]. The function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/> satisfying Equation (16) in this case is given by</p>
        <p><disp-formula id="symmetry-04-00452-i110"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i110.tif"/><label>(19)</label></disp-formula></p>
        <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i111.tif"/> are solutions of the equation <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i112.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i113.tif"/> is an arbitrary periodic function of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i114.tif"/> with period <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i105.tif"/>.</p>
        <p>• Other choices of parameters follow from more complicated choices for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i115.tif"/>. For example taking</p>
        <p><disp-formula id="symmetry-04-00452-i116"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i116.tif"/><label>(20)</label></disp-formula></p>
        <p>we obtain the change of parameters: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i117.tif"/>. </p>
        <p>Now, let us get back to the building of the potential algebra. In terms of operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i093.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/>, the shape invariance condition (12) becomes:</p>
        <p><disp-formula id="symmetry-04-00452-i118"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i118.tif"/><label>(21)</label></disp-formula></p>
        <p>Thus, the commutation relation of operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i119.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i120.tif"/> generates an operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i121.tif"/> that has no <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>-dependence. If we now define a third operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/> in terms of the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i124.tif"/>, the shape invariance condition becomes simply one of the commutation relations of the potential algebra. In particular, if we define</p>
        <p><disp-formula id="symmetry-04-00452-i125"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i125.tif"/><label>(22)</label></disp-formula></p>
        <p>where  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i105.tif"/> is an arbitrary constant, the three commutators among these generators are given by [<xref ref-type="bibr" rid="B39-symmetry-04-00452">39</xref>]</p>
        <p><disp-formula id="symmetry-04-00452-i126"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i126.tif"/><label>(23)</label></disp-formula></p>
        <p>Putting together the above results, we arrive at the following</p>
        <p>Lemma: <italic>To any shape invariant system characterized by</italic></p>
        <p><disp-formula id="symmetry-04-00452-i127"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i127.tif"/><label>(24)</label></disp-formula></p>
        <p><italic>for which we can find a function</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/><italic>such that</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i128.tif"/><italic>for arbitrary parameters</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i114.tif"/><italic>and</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i084.tif"/><italic>, we can associate an algebra</italic> [<xref ref-type="bibr" rid="B40-symmetry-04-00452">40</xref>]<italic>generated by</italic></p>
        <p><disp-formula id="symmetry-04-00452-i129"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i129.tif"/><label>(25)</label></disp-formula></p>
        <p><disp-formula id="symmetry-04-00452-i130"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i130.tif"/><label>(26)</label></disp-formula></p>
        <p><disp-formula id="symmetry-04-00452-i131"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i131.tif"/><label>(27)</label></disp-formula></p>
        <p>
          <italic>satisfying the commutation relations</italic>
        </p>
        <p><disp-formula id="symmetry-04-00452-i132"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i132.tif"/><label>(28)</label></disp-formula></p>
        <p><italic>where</italic></p>
        <p><disp-formula id="symmetry-04-00452-i133"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i133.tif"/><label>(29)</label></disp-formula></p>
        <p><italic>The function</italic>  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i134.tif"/><italic>in Equation (29) is given by the shape invariance condition (24), while the function</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/><italic>satisfies the compatibility equation:</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i135.tif"/><italic>, where</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i052.tif"/><italic>models the change of parameter</italic> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i079.tif"/><italic> of Equation (24).</italic></p>
        <p>As an example let us build the potential algebra corresponding to the Pöschl-Teller II potential. The potential</p>
        <p><disp-formula id="symmetry-04-00452-i136"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i136.tif"/><label>(30)</label></disp-formula></p>
        <p>is generated by the superpotential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i137.tif"/>, through <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i138.tif"/>, where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i139.tif"/>. Its supersymmetric partner <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i140.tif"/> is given by</p>
        <p><disp-formula id="symmetry-04-00452-i141"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i141.tif"/><label>(31)</label></disp-formula></p>
        <p>The shape invariance is now evident if we observe that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i142.tif"/>. Therefore, in terms of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i032.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i031.tif"/> operators, the shape invariance (24) for the Pöschl-Teller II potential reads</p>
        <p><disp-formula id="symmetry-04-00452-i143"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i143.tif"/><label>(32)</label></disp-formula></p>
        <p>Now we can identify the main objects of our model and build the corresponding algebra:</p>
        <p>1. The parameters of the model are <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i144.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i145.tif"/>, where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i146.tif"/> is an arbitrary positive constant greater than <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i147.tif"/> so that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i088.tif"/> is a positive quantity; </p>
        <p>2. The change of parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i079.tif"/> is thus given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i148.tif"/>. This is a translational change of parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i149.tif"/> with the translation parameter <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i150.tif"/>. Translation implies that the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i087.tif"/> satisfying (16) is the identity function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i098.tif"/>;</p>
        <p>3. From the concrete shape invariance condition (32) of this potential we get <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i151.tif"/>. Then, the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i152.tif"/> is given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i153.tif"/> if we choose the arbitrary constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i154.tif"/>;</p>
        <p>4. Defining <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i155.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/> as prescribed by Equations (25) and (27), we obtain the differential realization of the algebra’s generators:</p>
        <p><disp-formula id="symmetry-04-00452-i156"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i156.tif"/><label>(33)</label></disp-formula></p>
        <p>satisfying the commutation relations <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i157.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i158.tif"/>. Thus, shape invariance of this system implies that the system has a potential algebra given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i159.tif"/>[?, 41, 42]. </p>
      </sec>
      <sec>
        <title>4.2. Obtaining the Energy Spectrum from Algebra Representations</title>
        <p>Once we know the potential algebra for a given potential, we can use its representations to obtain the energy spectrum for the Hamiltonian. Using Equations (25) and (26), we observe that</p>
        <p><disp-formula id="symmetry-04-00452-i160"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i160.tif"/><label>(34)</label></disp-formula></p>
        <p>From the reciprocal of the mapping Equation (13), we obtain <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i161.tif"/>. Consequently, the spectrum of the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i162.tif"/> gives the spectrum of the Hamiltonian. To find the concrete values for the energy, we need to know the action of individual operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i093.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/> respectively on a set of eigenvectors of the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/>. In this general case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i093.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/> commute with the Casimir operator given by</p>
        <p><disp-formula id="symmetry-04-00452-i163"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i163.tif"/><label>(35)</label></disp-formula></p>
        <p>with the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i164.tif"/>(defined up to an additive constant) such that</p>
        <p><disp-formula id="symmetry-04-00452-i165"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i165.tif"/><label>(36)</label></disp-formula></p>
        <p>It can be explicitly checked that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i166.tif"/> does indeed commute with <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i093.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i090.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/>[<xref ref-type="bibr" rid="B41-symmetry-04-00452">41</xref>]. In a basis in which <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i166.tif"/> are diagonal, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i155.tif"/> play the role of raising and lowering operators, respectively. Operating on an arbitrary eigenstate <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i167.tif"/> we have</p>
        <p><disp-formula id="symmetry-04-00452-i168"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i168.tif"/><label>(37)</label></disp-formula></p>
        <p>where we have used <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i169.tif"/>.</p>
        <p>Keeping in mind that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i170.tif"/>, and observing that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i171.tif"/>, we see that in order to find the energies of the system one must find the coefficients <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i172.tif"/>. If we apply the third commutation relation of Equation (23) to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i167.tif"/>, we obtain using Equation (36) </p>
        <p><disp-formula id="symmetry-04-00452-i173"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i173.tif"/><label>(38)</label></disp-formula></p>
        <p>Next, we will determine the allowed values of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i174.tif"/> and the corresponding values <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i172.tif"/>. Let us say <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i175.tif"/> corresponds to the lowest state in a given representation of the algebra. This implies that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i176.tif"/>, which means <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i177.tif"/>. From Equation (38) we get</p>
        <p><disp-formula id="symmetry-04-00452-i178"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i178.tif"/><label>(39)</label></disp-formula></p>
        <p>Iterating this procedure we can generate a general formula for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i172.tif"/></p>
        <p><disp-formula id="symmetry-04-00452-i179"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i179.tif"/><label>(40)</label></disp-formula></p>
        <p>Substituting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i180.tif"/> leads to</p>
        <p><disp-formula id="symmetry-04-00452-i181"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i181.tif"/><label>(41)</label></disp-formula></p>
        <p>The profile of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/> determines the dimension of the representation. For example, let us consider the two cases presented in <xref ref-type="fig" rid="symmetry-04-00452-f001">Figure 1</xref>. </p>
        <fig id="symmetry-04-00452-f001" position="anchor">
          <label>Figure 1</label>
          <caption>
            <p>Generic behaviors of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/>. Case (<bold>a</bold>) corresponds to a finite, and (<bold>b</bold>) to an infinite representation of the potential algebra.</p>
          </caption>
          <graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-g001.tif"/>
        </fig>
        <p>One obtains the finite dimensional representations of <xref ref-type="fig" rid="symmetry-04-00452-f001">Figure 1</xref>a, by starting from a point on the <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/><italic>vs</italic>. <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i174.tif"/> graph corresponding to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i175.tif"/>, and moving in integer steps parallel to the <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i174.tif"/>-axis to the point corresponding to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i185.tif"/>. At the end points, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i186.tif"/>, and we get a finite representation. If <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/> is decreasing monotonically, as in <xref ref-type="fig" rid="symmetry-04-00452-f001">Figure 1</xref>b, there exists only one end point at <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i175.tif"/>. Starting from <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i187.tif"/> the value of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i174.tif"/> can be increased in integer steps up to infinity. In this case we have an infinite dimensional representation. As in the finite case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i187.tif"/> labels the representation. The difference is that here <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i187.tif"/> takes continuous values. Similar arguments apply for a monotonically increasing function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/>. Having the representation of the algebra associated with a characteristic model, we obtain, using Equation (41), the complete spectrum of the system.</p>
        <p>For example, let us consider the scaling change of parameters <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i188.tif"/>. Consider the simple choice <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i189.tif"/>, where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i190.tif"/> is a constant. This choice generates self-similar potentials studied in references [<xref ref-type="bibr" rid="B44-symmetry-04-00452">44</xref>,<xref ref-type="bibr" rid="B26-symmetry-04-00452">26</xref>,<xref ref-type="bibr" rid="B25-symmetry-04-00452">25</xref>]. In this case, combining Equation (18) with Equation (28) yields:</p>
        <p><disp-formula id="symmetry-04-00452-i191"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i191.tif"/><label>(42)</label></disp-formula></p>
        <p>which is a deformation of the standard <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i192.tif"/> Lie algebra.</p>
        <p>For this case, from Equations (42) and (36) one gets</p>
        <p><disp-formula id="symmetry-04-00452-i193"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i193.tif"/><label>(43)</label></disp-formula></p>
        <p>Note that for scaling problems [<xref ref-type="bibr" rid="B25-symmetry-04-00452">25</xref>], one requires <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i194.tif"/>, which leads to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i195.tif"/>. From the monotonically decreasing profile of the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i182.tif"/>, it follows that the unitary representations of this algebra are infinite dimensional. If we label the lowest weight state of the operator <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i123.tif"/> by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i187.tif"/>, then <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i177.tif"/>. Without loss of generality we can choose the coefficients <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i172.tif"/> to be real. Then one obtains from (38) for an arbitrary <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i196.tif"/></p>
        <p><disp-formula id="symmetry-04-00452-i197"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i197.tif"/><label>(44)</label></disp-formula></p>
        <p>The spectrum of the Hamiltonian <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i061.tif"/> is given by</p>
        <p><disp-formula id="symmetry-04-00452-i198"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i198.tif"/><label>(45)</label></disp-formula></p>
        <p>Therefore, the eigenenergies are</p>
        <p><disp-formula id="symmetry-04-00452-i199"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i199.tif"/><label>(46)</label></disp-formula></p>
        <p>in agreement with the known results [<xref ref-type="bibr" rid="B25-symmetry-04-00452">25</xref>].</p>
      </sec>
    </sec>
    <sec id="sec5-symmetry-04-00452">
      <title>5. How Do We Find Additive Shape Invariant Superpotentials?</title>
      <p>Since we have demonstrated the value of shape-invariant superpotentials, the question now becomes how to find such superpotentials. This question is equivalent to asking how to solve the difference-differential Equation (9) to find the list of desired superpotentials <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/>. For this section, we will restrict ourselves to considering cases of translational shape invariance. Before we embark on solving this equation, let us first note that quantum mechanical potentials generally have terms of two very different orders: One “large" and another “small". For example, the classical and quantum potentials for the radial oscillator system are <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i201.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i202.tif"/> respectively. To make the transition from the quantum to the classical system, one takes the limit <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i203.tif"/> with the constraint that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i204.tif"/>. Thus, the quantum Hamiltonian can be written as <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i205.tif"/>. This shows that in quantum mechanics, the potential generally has one small term that depends on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>[<xref ref-type="bibr" rid="B43-symmetry-04-00452">43</xref>]. In SUSYQM, since the potential is given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i206.tif"/>, the derivative term always brings in a factor of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, even if the superpotential is independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>. In the following analysis, as we determine how to solve Equation (9) to find shape invariant superpotentials, we will consider the cases of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-dependent superpotentials separately.</p>
      <sec>
        <title>5.1. Known  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i001.tif"/>-Independent Shape Invariant Superpotentials</title>
        <p>We begin our discussion of known shape invariant systems by considering only superpotentials that do not depend explicitly on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, which we call “conventional” superpotentials. In <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref> we list the known “conventional" superpotentials that meet this criterion.</p>
        <p>Previous work [<xref ref-type="bibr" rid="B45-symmetry-04-00452">45</xref>,<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>,<xref ref-type="bibr" rid="B47-symmetry-04-00452">47</xref>] has proven that this list of conventional shape-invariant superpotentials is complete. We now show a new proof of this completeness which has the advantage of being significantly more straightforward and elegant than it predecessors.</p>
        <table-wrap id="symmetry-04-00452-t001" position="anchor">
          <object-id pub-id-type="pii">symmetry-04-00452-t001_Table 1</object-id>
          <label>Table 1</label>
          <caption>
            <p>The complete family of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i001.tif"/>-independent additive shape-invariant superpotentials.</p>
          </caption>
          <table>
            <thead>
              <tr>
                <th align="left" valign="middle">Name </th>
                <th align="left" valign="middle">Superpotential </th>
              </tr>
            </thead>
            <tbody>
              <tr>
                <td align="left" valign="middle">Harmonic Oscillator </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i208.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Coulomb </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i209.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">-D oscillator </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i210.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Morse </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i211.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Rosen-Morse I </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i212.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Rosen-Morse II </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i213.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Eckart </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i214.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Scarf I </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i215.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Scarf II </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i216.tif"/></td>
              </tr>
              <tr>
                <td align="left" valign="middle">Gen. Pöschl-Teller </td>
                <td align="left" valign="middle"> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i217.tif"/></td>
              </tr>
            </tbody>
          </table>
        </table-wrap>
      </sec>
      <sec>
        <title>5.2. New Proof of Completeness of the Conventional Shape-Invariant Superpotentials</title>
        <p>Because of additive shape invariance, the dependence of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/> is through the linear combination <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i219.tif"/>; therefore, the derivatives of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> with respect to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/> are related by: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i220.tif"/>. Since Equation (7) must hold for an arbitrary value of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, if we assume that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> does not depend explicitly on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, we can expand in powers of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, and the coefficient of each power must separately vanish. Expanding the right hand side in powers of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/> yields </p>
        <p><disp-formula id="symmetry-04-00452-i221"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i221.tif"/><label>(47)</label></disp-formula></p>
        <p><disp-formula id="symmetry-04-00452-i222"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i222.tif"/><label>(48)</label></disp-formula></p>
        <p><disp-formula id="symmetry-04-00452-i223"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i223.tif"/><label>(49)</label></disp-formula></p>
        <p>Thus, all conventional additive shape invariant superpotentials are solutions of the above set of non-linear partial differential equations [<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>,<xref ref-type="bibr" rid="B47-symmetry-04-00452">47</xref>]. Although this represents an infinite set, note that if equations of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i224.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i225.tif"/> are satisfied, all others automatically follow. Therefore, we proceed to find all possible solutions to the two partial differential equations: </p>
        <p><disp-formula id="symmetry-04-00452-i226"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i226.tif"/><label>(50)</label></disp-formula></p>
        <p>and </p>
        <p><disp-formula id="symmetry-04-00452-i227"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i227.tif"/><label>(51)</label></disp-formula></p>
        <p>In doing so, we derive a new proof that the superpotentials shown in <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref> are the only possible solutions.</p>
        <p>The general solution to Equation (51) is</p>
        <p><disp-formula id="symmetry-04-00452-i228"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i228.tif"/><label>(52)</label></disp-formula></p>
        <p>Therefore, to generate all shape invariant superpotentials, we need to determine all possible combinations of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i229.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i230.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i231.tif"/> that satisfiy Equation (50). We will ignore the case when both <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i230.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i231.tif"/> are constants, as this corresponds to a flat potential with no  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>-dependence. We will also ignore the case in which <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i230.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i231.tif"/> are linearly dependent on each other; <italic>i.e.</italic>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i232.tif"/>. In this case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i233.tif"/>. If we redefine <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i234.tif"/>, this case becomes equivalent to a superpotential with a shifted parameter and constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> which will be considered shortly. We can therefore assume that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> are linearly independent of each other without loss of generality. Note that from here onward, we will use lower case Greek letters to denote constants that are independent of both <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>.</p>
        <p>To determine <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i010.tif"/>, we first focus on determining <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i229.tif"/>. To do so, we take two derivatives of (50) with respect to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/>. This leads to the following differential equation:</p>
        <p><disp-formula id="symmetry-04-00452-i237"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i237.tif"/><label/></disp-formula></p>
        <p>where dots and primes represent derivatives taken with respect to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/> respectively. Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i227.tif"/>, this simplifies to: </p>
        <p><disp-formula id="symmetry-04-00452-i238"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i238.tif"/><label>(53)</label></disp-formula></p>
        <p>Inserting the form of the general solution (52) into (53) yields</p>
        <p><disp-formula id="symmetry-04-00452-i239"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i239.tif"/><label>(54)</label></disp-formula></p>
        <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i240.tif"/> is a function of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/>, and is independent of  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>. Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> are linearly independent, we find that there are only three possible ways for the left-hand-side of Equation (54) to be independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>:</p>
        <p> • Case 1: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> is a constant and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i241.tif"/>; </p>
        <p> • Case 2: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> is a constant and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i242.tif"/>; </p>
        <p> • Case 3: Neither <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> nor <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> are not constants, but <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i242.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i241.tif"/>. </p>
        <p>For each of these cases we can determine the form of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i229.tif"/>. Then we can determine <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i230.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i231.tif"/> for these three cases. This we do by taking two derivatives of (50), this time one with respect to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and another with respect to  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>. This yields:</p>
        <p><disp-formula id="symmetry-04-00452-i243"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i243.tif"/><label>(55)</label></disp-formula></p>
        <p>Inserting the form of the general solution (52) into (55) yields</p>
        <p><disp-formula id="symmetry-04-00452-i244"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i244.tif"/><label>(56)</label></disp-formula></p>
        <p>Now, we will analyze each of the three cases in detail. </p>
        <sec>
          <title>5.2.1. Case 1: X1 Is a Constant and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i245.tif"/></title>
          <p>Let <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i246.tif"/>. Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> cannot be a constant as well, Equation (54) requires <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i241.tif"/>. This leads to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i247.tif"/> for some arbitrary constants <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i146.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i248.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i249.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i250.tif"/>. Inserting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i251.tif"/> into Equation (52) yields <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i252.tif"/> where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i253.tif"/>.</p>
          <p>We now find <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> by inserting the above <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> into Equation (50). This yields</p>
          <p><disp-formula id="symmetry-04-00452-i254"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i254.tif"/><label/></disp-formula></p>
          <p>or equivalently, </p>
          <p><disp-formula id="symmetry-04-00452-i255"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i255.tif"/><label>(57)</label></disp-formula></p>
          <p>where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i256.tif"/>.</p>
          <p>Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i231.tif"/> is independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/>, and the left side of (57) is a sum of four linearly independent functions of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i257.tif"/>, and the term <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i258.tif"/> on the right-hand-side is independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>, the coefficient of each power of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> must separately be independent of  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>. The linear term in <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> therefore requires that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i259.tif"/> be independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>. Since a constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> leads to a trivial solution, we must have <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i260.tif"/> The remaining <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>-dependent terms on the left side of (57), <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i261.tif"/> must be a constant:</p>
          <p><disp-formula id="symmetry-04-00452-i262"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i262.tif"/><label>(58)</label></disp-formula></p>
          <p>The solution depends on the value of the constants <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i052.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i263.tif"/>. </p>
          <p> • Case 1A: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i264.tif"/> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i265.tif"/> In this case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i266.tif"/>, which is a trivial solution; </p>
          <p> • Case 1B: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i264.tif"/> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i267.tif"/> In this case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i268.tif"/> so <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i269.tif"/> Defining <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i270.tif"/> yields the harmonic oscillator superpotential; </p>
          <p> • Case 1C: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i271.tif"/> The solution is then <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i272.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i273.tif"/> <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i246.tif"/>. Therefore, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i274.tif"/> For <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i275.tif"/>, this yields <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i276.tif"/>, where <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i277.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i278.tif"/>. This is the Morse superpotential. Note that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i279.tif"/> decreases as <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> increases, and hence signals a finite number of eigenstates [<xref ref-type="bibr" rid="B48-symmetry-04-00452">48</xref>]. </p>
        </sec>
        <sec>
          <title>5.2.2. Case 2: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i280.tif"/> Is Constant</title>
          <p>In this case, let <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i281.tif"/>; then Equation (54) requires <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i242.tif"/>. This yields <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i282.tif"/>. We now insert this form of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i251.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i281.tif"/> into (56) to get an ordinary differential equation in  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/> for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/>:</p>
          <p><disp-formula id="symmetry-04-00452-i283"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i283.tif"/><label/></disp-formula></p>
          <p>or equivalently, </p>
          <p><disp-formula id="symmetry-04-00452-i284"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i284.tif"/><label/></disp-formula></p>
          <p>Integrating it once, we get </p>
          <p><disp-formula id="symmetry-04-00452-i285"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i285.tif"/><label>(59)</label></disp-formula></p>
          <p>This equation can be simplified by setting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i286.tif"/>. This leads to </p>
          <p><disp-formula id="symmetry-04-00452-i287"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i287.tif"/><label>(60)</label></disp-formula></p>
          <p>The solutions for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i288.tif"/> depend on the constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i289.tif"/>.</p>
          <p>• Case 2A: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i290.tif"/> In this case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i291.tif"/> The whole superpotential is then given by </p>
          <p><disp-formula id="symmetry-04-00452-i292"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i292.tif"/><label>(61)</label></disp-formula></p>
          <p>Setting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i293.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i294.tif"/>, and identifying <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i295.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i296.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i297.tif"/>, we get <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i298.tif"/>: the superpotential for Coulomb [<xref ref-type="bibr" rid="B49-symmetry-04-00452">49</xref>];</p>
          <p> • Case 2B: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i299.tif"/> In this case, we have either <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i300.tif"/>(Eckart) or <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i301.tif"/>(Rosen-Morse II). In the first case, the superpotential is given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i302.tif"/>, where we have set <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i303.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i304.tif"/>. This is the well known Eckart potential. Similarly, the other solution with <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i305.tif"/> generates Rosen-Morse II;</p>
          <p> • Case 2C: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i306.tif"/> In this case, we obtain <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i307.tif"/>. An analysis similar to the previous case generates the superpotential for Rosen-Morse I. </p>
        </sec>
        <sec>
          <title>5.2.3. Case 3: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i308.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i280.tif"/> Are not Constant, but <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i309.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i245.tif"/></title>
          <p>In this case, since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i241.tif"/>, and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i242.tif"/>, we have <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i310.tif"/>. Therefore <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i311.tif"/>. In this case, Equation (56) yields</p>
          <p><disp-formula id="symmetry-04-00452-i312"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i312.tif"/><label/></disp-formula></p>
          <p>Integrating, </p>
          <p><disp-formula id="symmetry-04-00452-i285b"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i285b.tif"/><label>(62)</label></disp-formula></p>
          <p>Thus, again we have </p>
          <p><disp-formula id="symmetry-04-00452-i287b"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i287b.tif"/><label>(63)</label></disp-formula></p>
          <p>Note that this is the same differential equation as (60) and will therefore give the same solutions for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i236.tif"/> as Case 2. However, in this case, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i313.tif"/>(this is equivalent to choosing <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i314.tif"/> in Case 2) and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> is not constant. Instead, in each case we must plug our solutions for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i229.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i230.tif"/> into Equation (50), which yields</p>
          <p><disp-formula id="symmetry-04-00452-i315"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i315.tif"/><label/></disp-formula></p>
          <p>This equation is again simplified by setting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i286.tif"/>, which yields </p>
          <p><disp-formula id="symmetry-04-00452-i316"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i316.tif"/><label/></disp-formula></p>
          <p>Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i288.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> are independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/>, the terms linear in <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> and the terms independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> on the left side of this equation must each separately be independent of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>. Therefore, </p>
          <p><disp-formula id="symmetry-04-00452-i317"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i317.tif"/><label>(64)</label></disp-formula></p>
          <p><disp-formula id="symmetry-04-00452-i318"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i318.tif"/><label>(65)</label></disp-formula></p>
          <p>For different values of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i289.tif"/>, we get different superpotentials: </p>
          <p>• Case 3A: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i319.tif"/>. We again get <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i320.tif"/>, where with an appropriate choice for the origin we have set <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i294.tif"/>. Equation (65) for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i235.tif"/> becomes</p>
          <p><disp-formula id="symmetry-04-00452-i321"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i321.tif"/><label>(66)</label></disp-formula></p>
          <p> Its solution is <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i322.tif"/>. With the identification <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i323.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i324.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i325.tif"/>, we get <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i326.tif"/>, the superpotential for the 3D-harmonic oscillator; </p>
          <p>• Case 3B: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i299.tif"/> As seen before, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i327.tif"/> implies that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i300.tif"/> or <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i301.tif"/>. By translation and scaling of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i122.tif"/>, we can simplify the first solution to <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i328.tif"/>. Substituting <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i288.tif"/> in Equation (65), we get</p>
          <p><disp-formula id="symmetry-04-00452-i329"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i329.tif"/><label>(67)</label></disp-formula></p>
          <p>where we have set <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i330.tif"/> The solution to the homogeneous equation is <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i331.tif"/>, and the particular solution is <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i332.tif"/>. Hence <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i333.tif"/>. Thus, the superpotential is given by <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i334.tif"/>, the General Pöschl-Teller potential given in <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref>. The second solution generates the Scarf II potential;</p>
          <p> • Case 3C: <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i306.tif"/> A similar analysis for this case leads to Scarf I as the corresponding shape invariant superpotential. </p>
          <p>Thus, we have generated all the superpotentials of <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref> and shown that these are the only possible <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent solutions to the additive shape invariant condition.</p>
        </sec>
      </sec>
      <sec>
        <title>5.3.  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i001.tif"/>-Dependent Superpotentials</title>
        <p>In the previous section we generated the complete list of additive shape-invariant superpotentials that do not depend explicitly on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>. However, a new class of superpotentials was discovered by Quesne [<xref ref-type="bibr" rid="B50-symmetry-04-00452">50</xref>,<xref ref-type="bibr" rid="B51-symmetry-04-00452">51</xref>]. It has been shown [<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>] that these “extended" superpotentials obey the shape invariance condition in the form of Equation (7) only when  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> is allowed to depend explicitly on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>. While this dependence is frequently ignored by the conventional notation that sets <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i335.tif"/>, we will show that this constraint results in important consequences for the energy spectrum of the resulting potentials. In each case, the new potential is isospectral with a potential that arises from one of the “conventional" superpotentials listed in <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref>. Authors of [<xref ref-type="bibr" rid="B52-symmetry-04-00452">52</xref>,<xref ref-type="bibr" rid="B53-symmetry-04-00452">53</xref>,<xref ref-type="bibr" rid="B54-symmetry-04-00452">54</xref>] have added an infinite number of potentials that belong in this class, and extended shape invariant potentials continue to be objects of intense research [<xref ref-type="bibr" rid="B55-symmetry-04-00452">55</xref>,<xref ref-type="bibr" rid="B56-symmetry-04-00452">56</xref>].</p>
        <p>We now extend our formalism to include “extended" superpotentials that contain <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/> explicitly. To do so, we expand the superpotentials in powers of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>. Hence, we define </p>
        <p><disp-formula id="symmetry-04-00452-i336"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i336.tif"/><label>(68)</label></disp-formula></p>
        <p>We will now substitute Equation (68) into the shape invariance condition given in Equation (7), for which we compute <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i337.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i338.tif"/>. We obtain</p>
        <p><disp-formula id="symmetry-04-00452-i339"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i339.tif"/><label/></disp-formula></p>
        <p>and </p>
        <p><disp-formula id="symmetry-04-00452-i340"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i340.tif"/><label/></disp-formula></p>
        <p>Since <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i148.tif"/>, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i341.tif"/> Expanding in powers of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i342.tif"/></p>
        <p><disp-formula id="symmetry-04-00452-i343"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i343.tif"/><label/></disp-formula></p>
        <p>Similarly, </p>
        <p><disp-formula id="symmetry-04-00452-i344"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i344.tif"/><label/></disp-formula></p>
        <p>We substitute these into Equation (7) and stipulate that the equation hold for any value of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>. After some significant algebraic manupulation we find that the following equation must be true separately for each positive integer value of  <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i345.tif"/>: </p>
        <p><disp-formula id="symmetry-04-00452-i346"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i346.tif"/><label>(69)</label></disp-formula></p>
        <p>For <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i347.tif"/>, we obtain </p>
        <p><disp-formula id="symmetry-04-00452-i348"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i348.tif"/><label>(70)</label></disp-formula></p>
        <p>This equation is identical to Equation (50) for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/>’s. We have already found a set of solutions for Equation (70) that includes all known <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent superpotentials. The extended cases [<xref ref-type="bibr" rid="B50-symmetry-04-00452">50</xref>,<xref ref-type="bibr" rid="B51-symmetry-04-00452">51</xref>] are solutions to (69) as well, as shown in [<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>]. Note that Equation (69) provides a consistency condition for all <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-dependent potentials; however, these are not easy to solve to determine new potentials.</p>
        <p>Additionally, Equation (70) provides a constraint for the possible energy spectra of the extended potentials. from Equation (70), the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i349.tif"/> is given by</p>
        <p><disp-formula id="symmetry-04-00452-i350"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i350.tif"/><label>(71)</label></disp-formula></p>
        <p><disp-formula id="symmetry-04-00452-i351"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i351.tif"/><label>(72)</label></disp-formula></p>
        <p>Thus, the function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i349.tif"/>, and hence the energy of the system, is given entirely in terms of the <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent part of the superpotential. Hence, the eigenvalues are not affected by the <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-dependent extension of the superpotential.</p>
        <p>Thus far, each of the known extended potentials contains a solution from <xref ref-type="table" rid="symmetry-04-00452-t001">Table 1</xref> as the <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent term of the superpotential <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i352.tif"/>. Therefore, each of the expanded potentials is isospectral with its corresponding conventional potential. Future possibilities for finding new shape-invariant superpotentials fall into one of two categories: </p>
        <p> 1. Further extended superpotentials may be found based on the conventional superpotentials. In this case, the potentials derived from the extended superpotential will be isospectral with the potentials derived from the corresponding conventional superpotential; </p>
        <p>2. While <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i352.tif"/> is required to satisfy Equation (70), which is equivalent to Equation (50) for <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/>’s, <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i352.tif"/> is not required to satisfy Equation (48). Rather, the additional constraints for an extended <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i200.tif"/> are supplied by Equation (69). It therefore may be possible to find an <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-dependent superpotential whose <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>-independent term <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i352.tif"/> is not equivalent to a conventional superpotential. Intriguingly, it therefore may still be possible to discover shape-invariant systems with new energy spectra.</p>
      </sec>
    </sec>
    <sec>
      <title>6. Summary and Conclusions</title>
      <p>While supersymmetric quantum mechanics began as a simplified model to account for dynamical symmetry breaking, the application of this formalism to quantum mechanics has become an important field in its own right. In this manuscript we have reviewed research on supersymmetric quantum mechanics with a particular emphasis on the property of shape invariance. As we have shown, shape invariance is a sufficient condition for exact solvability of quantum mechanical problems; <italic>i.e.</italic>, given a superpotential with shape invariance, all its eigenvalues and eigenfunctions can be determined analytically.</p>
      <p>However, in its traditional form, the shape invariance condition Equation (7) is a difference-differential equation and is difficult to solve. It has recently been established that for additive shape-invariant superpotentials that do not explicitly depend on <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>, this condition can be written as a set of local partial differential equations [<xref ref-type="bibr" rid="B45-symmetry-04-00452">45</xref>,<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>,<xref ref-type="bibr" rid="B47-symmetry-04-00452">47</xref>]. The solution to these equations showed that the list of such superpotentials was indeed complete. In this manuscript, we have presented a more straightforward proof of this result.</p>
      <p>Since 2008, new sets of additive shape invariant potentials have been discovered [<xref ref-type="bibr" rid="B50-symmetry-04-00452">50</xref>,<xref ref-type="bibr" rid="B51-symmetry-04-00452">51</xref>,<xref ref-type="bibr" rid="B52-symmetry-04-00452">52</xref>,<xref ref-type="bibr" rid="B53-symmetry-04-00452">53</xref>,<xref ref-type="bibr" rid="B54-symmetry-04-00452">54</xref>]. We have reviewed the development of these “extended" shape-invariant systems and have provided an infinite set of partial differential equations that all extended potentials (where superpotentials are inherently functions of <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i002.tif"/>) must obey [<xref ref-type="bibr" rid="B46-symmetry-04-00452">46</xref>,<xref ref-type="bibr" rid="B47-symmetry-04-00452">47</xref>]. We have also discussed the constraints placed on the energy spectra of these extended potentials as well as possibilities for finding additional as-yet-undiscovered cases of additive shape invariance.</p>
      <p>It may also be possible to extend this method to other forms of shape invariance such as multiplicative or cyclic. For these, the potentials are generally not available in terms of known functions, except in very special cases ( <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i353.tif"/> for cyclic and limiting cases for multiplicative). It remains to be shown whether the shape invariance condition for these classes can be transformed from a difference-differential equation into a set of partial differential equations and be subjected to similar analysis.</p>
    </sec>
  </body>
  <back>
    <ack>
      <title>Acknowledgements</title>
      <p>This research was supported by an award from Research Corporation for Science Advancement</p>
    </ack>
    <ref-list>
      <title>References and Notes</title>
      <ref id="B1-symmetry-04-00452">
        <label>1.</label>
        <citation citation-type="book">
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		<note><p>Note the constant <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i354.tif"/> has been added to the usual harmonic oscillator potential to insure that the groundstate energy of the system remains at zero. This constant allows us to factorize the Hamiltonian <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i013.tif"/> as a product of operators <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i032.tif"/> and <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i031.tif"/>.</p></note>
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		<note><p>We assume that as <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i359.tif"/>, the supersymmetry remains unbroken.</p></note>
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		<note><p>In the last line we have used the fact that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i360.tif"/>. This implies that for any analytical function <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i361.tif"/>, we have <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i362.tif"/>.</p></note>
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		<note><p>Normalizability of the groundstate <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i365.tif"/> requires that <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i279.tif"/> be greater than zero. Since an increase in <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i218.tif"/> decreases <inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="symmetry-04-00452-i279.tif"/>, there can only be a finite number of increases.</p></note>
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