<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJM</journal-id><journal-title-group><journal-title>Open Journal of Microphysics</journal-title></journal-title-group><issn pub-type="epub">2162-2450</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojm.2019.91001</article-id><article-id pub-id-type="publisher-id">OJM-90333</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Pseudo-Hermitian Matrix Exactly Solvable Hamiltonian
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ancilla</surname><given-names>Nininahazwe</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Institut de Pédagogie Appliquée, Université du Burundi, Bujumbura, Burundi</addr-line></aff><pub-date pub-type="epub"><day>30</day><month>01</month><year>2019</year></pub-date><volume>09</volume><issue>01</issue><fpage>1</fpage><lpage>9</lpage><history><date date-type="received"><day>9,</day>	<month>January</month>	<year>2019</year></date><date date-type="rev-recd"><day>28,</day>	<month>January</month>	<year>2019</year>	</date><date date-type="accepted"><day>31,</day>	<month>January</month>	<year>2019</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   The non PT-symmetric exactly solvable Hamiltonian describing a system of a fermion in the external magnetic field which couples to a harmonic oscillator through some pseudo-hermitian interaction is considered. We point out all properties of both of the original Mandal and the original Jaynes-Cummings Hamitonians. It is shown that these Hamiltonians are respectively pseudo-hermitian and hermitian  REF _Ref536606452 \r \h \* MERGEFORMAT [1]  REF _Ref536606454 \r \h [2]. Like the direct approach to invariant vector spaces used in Refs.  REF _Ref536606456 \r \h [3]  REF _Ref536606457 \r \h [4], we reveal the exact solvability of both the Mandal and Jaynes-Cummings Hamiltonians after expressing them in the position operator and the impulsion operator.  
  
 
</p></abstract><kwd-group><kwd>Pseudo-Hermiticity</kwd><kwd> Exact Solvability</kwd><kwd> Direct Method</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Several new theoretical aspects in quantum mechanics have been developed in last years. In the series of papers [<xref ref-type="bibr" rid="scirp.90333-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref6">6</xref>] , it is shown that the traditional self adjointness requirement (i.e. the hermiticity property) of a Hamilton operator is not necessary condition to guarantee real eigenvalues and that the weaker condition PT-symmetry of the Hamiltonian is sufficient for the purpose. Following the theory developed in Refs. [<xref ref-type="bibr" rid="scirp.90333-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref6">6</xref>] , let’s remind that a Hamiltonian is invariant under the action of the combined parity operator P and the time reversal operator T if the relation H P T = H is proved (i.e. PT-symmetry is said to be broken). As a consequence, the spectrum associated the previous Hamiltonian is entirely real.</p><p>An alternative property called pseudo-hermiticity for a Hamiltonian to be associated to a real spectrum is shown in details in the Refs. [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] .</p><p>Referring the ideas of [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] , we recall here that a Hamiltonian is said to be η pseudo-hermitian if it satisfies the relation η H η − 1 = H + , where η denotes an invertible linear hermitian operator.</p><p>Another direction of quantum mechanics is the notions of quasi exact solvability and exact solvability [<xref ref-type="bibr" rid="scirp.90333-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref10">10</xref>] .</p><p>In the last few years, a new class of operators has been discovered. This class is intermediate between exactly solvable operators and non solvable operators. Its name is the quasi-exactly solvable (QES) operators, for which a finite part of the spectrum can be computed algebraically.</p><p>This paper is organized as follows:</p><p>In Section 2, we briefly describe the general model which is expressed in terms of the creation and the annihilation operators. We show that the Hamiltonian describing the model is pseudo-hermitian if ϕ = − 1 , or it is hermitian if ϕ = + 1 .</p><p>In Section 3, we show in details the properties of the Mandal Hamiltonian namely the non-hermiticity, the non PT-symmetry, the pseudo-hermiticity and the exact solvability.</p><p>In Section 4, as in the previous section, it was pointed out that the original Jaynes-Cummings Hamiltonian is hermitian and exactly solvable.</p></sec><sec id="s2"><title>2. The Model</title><p>In this section, we consider a Hamiltonian describing a system of a fermion in the external magnetic field, B which couples the harmonic oscillator interaction (i.e. ℏ ω a + a ) and the pseudo-hermitian interaction if ϕ = − 1 , or the hermitian interaction if ϕ = + 1 (i.e.<inline-formula><inline-graphic xlink:href="/html.scirp.org/file/1-1220105x12.png" xlink:type="simple"/></inline-formula>) [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula1"><label>, (1)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x13.png"  xlink:type="simple"/></disp-formula><p>where</p><p>σ , σ &#177; denote Pauli matrices,</p><p>ρ , μ are real parameters,</p><p>a + , a refer the creation and annihilation operators respectively satisfying the usual bosonic commutation relation</p><p>[ a , a + ] = 1 , [ a , a ] = [ a + , a + ] = 0 and σ &#177; ≡ 1 2 ( σ x &#177; i σ y ) .</p><p>Recall that the matrices σ + , σ − , σ x , σ y and σ z can be expressed in the following matrix forms:</p><disp-formula id="scirp.90333-formula2"><label>(2)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x24.png"  xlink:type="simple"/></disp-formula><p>For the sake simplicity, one can choose the external field in the z-direction (i.e. B = B 0 z ) in order to reduce the Hamiltonian given by the Equation (1) and it becomes [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula3"><label>(3)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x26.png"  xlink:type="simple"/></disp-formula><p>with ε = 2 μ B 0 and ℏ = 1 .</p></sec><sec id="s3"><title>3. Properties of the Original Mandal Hamiltonian</title><sec id="s3_1"><title>3.1. The Non-Hermiticity</title><p>In this section, we reveal that the Hamiltonian described by the Equation (3) is non- hermitian if ϕ = − 1 . It is called Mandal Hamiltonian (i.e. H M ) and it takes the following form:</p><disp-formula id="scirp.90333-formula4"><label>(4)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x31.png"  xlink:type="simple"/></disp-formula><p>Taking account to the following identities:</p><disp-formula id="scirp.90333-formula5"><label>(5)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x32.png"  xlink:type="simple"/></disp-formula><p>let’s show that the Mandal Hamiltonian given by the above Equation (4) is non hermitian:</p><p>H M + = ( ε 2 σ z ) + + ( ω a + a ) + + [ ρ ( σ + a − σ − a + ) ] + ,</p><disp-formula id="scirp.90333-formula6"><label>. (6)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x34.png"  xlink:type="simple"/></disp-formula><p>Comparing the expressions given by the Equations (4) and (6), we see that they are different (i.e. H M + ≠ H M ), as a consequence, we are allowed to conclude that the Mandal Hamiltonian H M is non-hermitian.</p></sec><sec id="s3_2"><title>3.2. The Non PT-Symmetry of H<sub>M</sub></title><p>In this section, we prove that the Mandal Hamiltonian is non PT-symmetric [<xref ref-type="bibr" rid="scirp.90333-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref6">6</xref>] . Recall that the parity operator is represented by the symbol P and the time-reversal operator is described by the symbol T.</p><p>The effect of the parity operator P implies the following changes [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula7"><label>(7)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x37.png"  xlink:type="simple"/></disp-formula><p>Notice also the changes of the following quantities under the effect of the time reversal operator T:</p><disp-formula id="scirp.90333-formula8"><label>(8)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x38.png"  xlink:type="simple"/></disp-formula><p>Taking account to the relations (7) and (8), one can easily deduce the changes of the Mandal Hamiltonian under the effect of combined operators P et T as follows</p><p><inline-formula><inline-graphic xlink:href="/html.scirp.org/file/1-1220105x39.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.90333-formula9"><label>, (9)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x40.png"  xlink:type="simple"/></disp-formula><p>This above relation (9) can be written as follows</p><disp-formula id="scirp.90333-formula10"><label>(10)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x41.png"  xlink:type="simple"/></disp-formula><p>Comparing the relations (4) and (10), we see that they are different (i.e. H M P T ≠ H M ), it means that the Mandal Hamiltonian H M is not invariant under the combined action of the parity operator P and the time-reversal operator T. In other words, the Mandal Hamiltonian H M is not PT-symmetric.</p></sec><sec id="s3_3"><title>3.3. Pseudo-Hermiticity of H<sub>M</sub></title><p>In this section, we first prove that the non PT-symmetric Mandal Hamiltonian is pseudo-hermitian with respect to third Pauli matrix σ z [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula11"><label>(11)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x46.png"  xlink:type="simple"/></disp-formula><p>with σ z σ &#177; σ z − 1 = − σ ∓ and W n = e − ω x 2 2 ( P n − 1 ( x ) , P n ( x ) ) t .</p><p>Comparing the Equations (6) and (11), it is seen that the following relation is satisfied:</p><p>W n = e − ω x 2 2 ( P n − 1 ( x ) , P n ( x ) ) t (12)</p><p>Taking account to this above relation, we are allowed to conclude that the Mandal Hamiltonian is pseudo-hermitian with respect to σ z .</p><p>Finally, we reveal a pseudo-hermiticity of H M with respect to the parity operator P:</p><disp-formula id="scirp.90333-formula12"><label>(13)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x52.png"  xlink:type="simple"/></disp-formula><p>Here we have used the relations (7) in order to obtain this above equation (13). As a consequence, one can conclude that the Mandal Hamiltonian is pseudo-hermitian with respect to the parity operator P.</p><p>Note that even if H M is non hermitian and non PT-symmetric, its eigenvalues are entirely real due to the pseudo-hermiticity property [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] .</p></sec><sec id="s3_4"><title>3.4. Differential Form and Exact Solvability of H<sub>M</sub></title><p>In this step, our purpose is to change the Mandal Hamiltonian given by the Equation (4) in appropriate differential operator (i.e. H M is expressed in the position operator x and in the impulsion operator H J C + = ε 2 σ z + ω a + a + [ ρ ( σ + a + σ − a + ) ] ). Thus, referring to the ideas of exactly and quasi-exactly solvable operators studied in the Refs. [<xref ref-type="bibr" rid="scirp.90333-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref10">10</xref>] , we reveal that H M preserves a family of vector spaces of polynomials in the variable x.</p><p>With this aim, we use the usual representation of the creation and annihilation operators of the harmonic oscillator respectively a + and a [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula13"><label>(14)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x58.png"  xlink:type="simple"/></disp-formula><p>where ω is the oscillation frequency, m denotes the mass, x refers to the position operator and the impulsion operator is<inline-formula><inline-graphic xlink:href="/html.scirp.org/file/1-1220105x60.png" xlink:type="simple"/></inline-formula>, p 2 = − d 2 d x 2 .</p><p>Using appropriate units, we can assume m = ℏ = 1 and the operators a + and a take the following forms:</p><disp-formula id="scirp.90333-formula14"><label>(15)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x64.png"  xlink:type="simple"/></disp-formula><p>Replacing the operators a + and a by their expressions given by this above Equation (15) in the Equation (4), the Mandal Hamiltonian H M takes the following form:</p><disp-formula id="scirp.90333-formula15"><label>. (16)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x67.png"  xlink:type="simple"/></disp-formula><p>In order to reveal the exact solvability of the above operator H M , we first perform the standard gauge transformation [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] :</p><disp-formula id="scirp.90333-formula16"><label>(17)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x69.png"  xlink:type="simple"/></disp-formula><p>After some algebraic manipulations, the new Hamiltonian H ˜ M (known as gauge Hamiltonian) is obtained</p><disp-formula id="scirp.90333-formula17"><label>(18)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x71.png"  xlink:type="simple"/></disp-formula><p>Replacing the Pauli matrices <inline-formula><inline-graphic xlink:href="//html.scirp.org/file/1-1220105x72.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="//html.scirp.org/file/1-1220105x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="//html.scirp.org/file/1-1220105x73.png" xlink:type="simple"/></inline-formula> by their respective expressions given by the relation (2), the final form of the gauge Hamiltonian is:</p><p><inline-formula><inline-graphic xlink:href="//html.scirp.org/file/1-1220105x74.png" xlink:type="simple"/></inline-formula>,</p><disp-formula id="scirp.90333-formula18"><label>. (19)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x75.png"  xlink:type="simple"/></disp-formula><p>Note that one can easily check if this above gauge Hamiltonian H ˜ M preserves the vector spaces of polynomials <inline-formula><inline-graphic xlink:href="//html.scirp.org/file/1-1220105x77.png" xlink:type="simple"/></inline-formula> with n ∈ Ν . As the integer n doesn’t have to be fixed (i.e. it is arbitrary), H ˜ M is exactly solvable. Indeed, its all eigenvalues can be computed algebraically. Even if the gauge Mandal Hamiltonian H ˜ M is non-hermitian and non PT-symmetric, its spectrum energy is entirely real due to the property of the pseudo-hermiticity [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] .</p><p>Thus, the vector spaces preserved by the operator H M have the following form</p><disp-formula id="scirp.90333-formula19"><label>(20)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/1-1220105x82.png"  xlink:type="simple"/></disp-formula><p>where P n − 1 ( x ) and P n ( x ) denote respectively the polynomials of degree n − 1 and n.</p><p>As the gauge Mandal Hamiltonian H ˜ M , it is obvious that the original Mandal Hamiltonian H M is exactly solvable. Due to this property of exact solvability, the whole spectrum of H M can be computed exactly (i.e. by the algebraic methods) [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref3">3</xref>] .</p></sec></sec><sec id="s4"><title>4. Properties of the Jaynes-Cummings Hamiltonian</title><sec id="s4_1"><title>4.1. The Hermiticity</title><p>In this section, considering ϕ = + 1 , the Hamiltonian given by the Equation (3) leads to the standard Jaynes-Cummings Hamiltonian of the following form</p><p>H J C = ε 2 σ z + ω a + a + ρ ( σ + a + σ − a + ) (21)</p><p>Our aim is now to prove that the above Hamiltonian H J C is hermitian.</p><p>Indeed, in order to reveal the hermiticity of the Jaynes-Cummings Hamiltonian given by the above relation (21), the following relation H J C + = H J C must be satisfied.</p><p>Consider now the following relation</p><p>H J C + = ( ε 2 σ z ) + + ( ω a + a ) + + [ ρ ( σ + a + σ − a + ) ] + , (22)</p><p>Taking account to the identities of the relation (5), this above equation leads the following expression:</p><p>H J C + = ε 2 σ z + ω a + a + [ ρ ( σ + a + σ − a + ) ] . (23)</p><p>Comparing the Equations (21) and (23), one can write that</p><p>H J C + = H J C . (24)</p><p>Referring to this equation (24), it is obvious that the standard Jaynes-Cummings Hamiltonian is hermitian. As a consequence, its eigenvalues are real due to the property of hermiticity.</p></sec><sec id="s4_2"><title>4.2. Differential Form and Exact Solvability of H<sub>JC</sub></title><p>Along the same lines as in the above section 3.4, our purpose is to change the Jaynes-Cummings Hamiltonian given by the Equation (21) in appropriate differential operator (i.e. H J C is expressed in the position operator x and in the impulsion operator p = − i d d x ).</p><p>With this purpose, we use the usual expressions of the creation and annihilation operators of the harmonic oscillator respectively a + and a given by the Equation (15).</p><p>Substituting (15) in the Equation (21), the Jaynes-Cummings Hamiltonian H J C is written now as follows</p><p>H J C = ε 2 σ z + p 2 − ω + ω 2 x 2 2 + ρ [ σ + ( p − i ω x ) + σ − ( p + i ω x ) ] 2 ω (25)</p><p>Operating on the above operator H J C the standard gauge transformation as</p><p>H ˜ J C = R − 1 H J C R ,       R = exp ( − ω x 2 2 ) , (26)</p><p>after some algebraic manipulations, the new Hamiltonian H ˜ J C (known as gauge Hamiltonian) is obtained</p><p>H ˜ M = ε 2 σ z − 1 2 d 2 d x 2 + ω x d d x + ρ [ σ + p + σ − ( p + 2 i ω x ) ] 2 ω = ε 2 σ z + p 2 2 + i ω x p + ρ [ σ + p + σ − ( p + 2 i ω x ) ] 2 ω (27)</p><p>Replacing the Pauli matrices σ z , σ + and σ − respectively by their matrix form given by the relation (2), the final form of the gauge Hamiltonian H ˜ J C is</p><p>H ˜ M = ε 2 ( 1 0 0 − 1 ) + ( p 2 2 + i ω x p 0 0 p 2 2 + i ω x p ) + ρ ( 0 p 2 ω p + 2 i ω x 2 ω 0 ) ,</p><p>H ˜ M = ( p 2 2 + i ω x p + ε 2 ρ p 2 ω ρ p + 2 i ω x 2 ω p 2 2 + i ω x p − ε 2 ) . (28)</p><p>Note that one can easily check if this above gauge Hamiltonian H ˜ J C preserves the finite dimensional vector spaces of polynomials namely V n = ( P n − 1 ( x ) , P n ( x ) ) t with n ∈ Ν . As the integer n is arbitrary, the gauge Jaynes-Cummings Hamiltonian H ˜ J C is exactly solvable.</p><p>As a consequence, its all eigenvalues can be computed algebraically. Indeed, the vector spaces preserved by the operator H J C have the following form</p><p>W n = e − ω x 2 2 ( P n − 1 ( x ) , P n ( x ) ) t (29)</p><p>where P n − 1 ( x ) and P n ( x ) denote respectively the polynomials of degree n − 1 and n.</p><p>As the gauge Jaynes-Cummings Hamiltonian H ˜ J C , it is obvious that the standard Jaynes-Cummings Hamiltonian H J C is exactly solvable. In other words, all eigenvalues associated to the Hamiltonian H J C can be calculated algebraically (i.e. by the algebraic methods) [1-3].</p></sec></sec><sec id="s5"><title>5. Conclusion</title><p>In this paper, we have put out all properties of the original Mandal Hamiltonian. We have shown that the Mandal Hamiltonian H M is non-hermitian and non-invariant under the combined action of the parity operator P and the time-reversal operator T. Even if the previous properties are not satisfied, it has been proved that the Mandal Hamiltonian H M is pseudo-hermitian with respect to P and with respect to σ 3 also. With the direct method, we have revealed that H M preserves the finite dimensional vector spaces of polynomials namely V n = ( P n − 1 ( x ) , P n ( x ) ) t . Indeed, the Mandal Hamiltonian H M is said to be exactly solvable [<xref ref-type="bibr" rid="scirp.90333-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.90333-ref4">4</xref>] . Along the same lines used in Section 3, we have pointed out that the standard Jaynes-Cummings Hamiltonian H J C is hermitian and exactly solvable in Section 4.</p></sec><sec id="s6"><title>Acknowledgements</title><p>I thank Pr. Yves Brihaye of useful discussions.</p></sec><sec id="s7"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s8"><title>Cite this paper</title><p>Nininahazwe, A. (2019) Pseudo-Hermitian Matrix Exactly Solvable Hamiltonian. Open Journal of Microphysics, 9, 1-9. https://doi.org/10.4236/ojm.2019.91001</p></sec></body><back><ref-list><title>References</title><ref id="scirp.90333-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Mandal, B.P. (2005) Pseudo-Hermitian Interaction between an Oscillator and a Spin   Particle in the External Magnetic Field. Modern Physics Letters A, 20, 655-662. https://doi.org/10.1142/S0217732305016488</mixed-citation></ref><ref id="scirp.90333-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Brihaye, Y. and Nininahazwe, A. (2006) Extended Jaynes-Cummings Models and Quasi-Exact Solvability. Journal of Physics A: Mathematical and General, 39, 1-14. https://doi.org/10.1088/0305-4470/39/31/011</mixed-citation></ref><ref id="scirp.90333-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Rühl, W. and Turbiner, A. (1995) Exact Solvability of the Calogero and the Sutherland Models. Modern Physics Letters A, 10, 2213. https://doi.org/10.1142/S0217732395002374</mixed-citation></ref><ref id="scirp.90333-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Gomez-Ullate, D., Kamran, N. and Milson, R. (2005) Quasi-Exact Solvability and the Direct Approach to Invariant Subspaces. Journal of Physics, A38, 2005-2019.https://doi.org/10.1088/0305-4470/38/9/011</mixed-citation></ref><ref id="scirp.90333-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Bender, C. and Boettcher, S. (1998) Real Spectra in Non-Hermitian Hamiltonians having PT-Symmetry. Physical Reviews Letters, 80, 5243.https://doi.org/10.1103/PhysRevLett.80.5243</mixed-citation></ref><ref id="scirp.90333-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Brihaye, Y. and Nininahazwe, A. (2004) On PT-Symmetric Extensions of the Calogero and the Sutherland Models. International Journal of Morden Physics, A19, 4391-4400. https://doi.org/10.1142/S0217751X04019858</mixed-citation></ref><ref id="scirp.90333-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Turbiner, A.V. (1988) Quasi-Exactly Solvable Problems and sl(2) Algebra. Communications in Mathematical Physics, 118, 467-474.https://doi.org/10.1007/BF01466727</mixed-citation></ref><ref id="scirp.90333-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Ushveridze, A.G. (1995) Quasi-Exactly Solvable Models in Quantum Mechanics. Institute of Physics Publishing.</mixed-citation></ref><ref id="scirp.90333-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Brihaye, Y. and Kosinski, P. (1997) Quasi-Exactly Solvable Matrix Models in sl(n). Physics Letters B, 424, 43-47. https://doi.org/10.1016/S0370-2693(98)00167-1</mixed-citation></ref><ref id="scirp.90333-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Brihaye, Y. and Hartmann, B. (2001) Quasi-Exactly Solvable  -Matrix Schr&amp;#246;dinger Operators. Modern Physics Letters A, 16, 1895-1906.https://doi.org/10.1142/S0217732301005242</mixed-citation></ref></ref-list></back></article>