<?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.2013.33011</article-id><article-id pub-id-type="publisher-id">OJM-35704</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>
 
 
  Calogero Model with Different Masses
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ncilla</surname><given-names>Nininahazwe</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Université du Burundi, Institut de Pédagogie Appliquée, Bujumbura, Burundi</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>nininaha@yahoo.fr</email></corresp></author-notes><pub-date pub-type="epub"><day>09</day><month>08</month><year>2013</year></pub-date><volume>03</volume><issue>03</issue><fpage>60</fpage><lpage>63</lpage><history><date date-type="received"><day>May</day>	<month>15,</month>	<year>2013</year></date><date date-type="rev-recd"><day>June</day>	<month>15,</month>	<year>2013</year>	</date><date date-type="accepted"><day>June</day>	<month>22,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  We study a multispecies one-dimensional Calogero model with two-
   
  and three-body interactions. Here, we factorize the ground state<inline-formula><inline-graphic xlink:href="dit_daf21f77-00d7-4ca9-8efc-60825f171af9.png" xlink:type="simple"/></inline-formula>
  out of the Hamiltonian 
  H
   in order to get the new operator<inline-formula><inline-graphic xlink:href="dit_689630e3-4393-40f2-bfb5-ec3b5ffe33a6.png" xlink:type="simple"/></inline-formula>which preserves some spaces of polynomials<inline-formula><inline-graphic xlink:href="dit_96560345-e33e-44fc-90d1-0dabf6e4e1bf.png" xlink:type="simple"/></inline-formula>in the case of equal masses, i.e
  .<inline-formula><inline-graphic xlink:href="dit_4e1e4e18-ae61-450f-b507-d3913499af13.png" xlink:type="simple"/></inline-formula>
    (the usual Calogero model) and in the case with different masses. The spectrum of these both cases is found easily.
 
</p></abstract><kwd-group><kwd>Multispecies One-Dimensional Calogero; Equal Masses; Different Masses; Usual Calogero Model</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The ordinary Cologero [1,2] model describes N indistinguishable particles on the line which interact through an inverse-square two-body interaction. The model is completely integrable in both the classical and quantum case [<xref ref-type="bibr" rid="scirp.35704-ref3">3</xref>]. The spectrum is known and the wave functions are given implicitly. In the present paper, which is in a sense a continuation of the investigation of the ordinary model [<xref ref-type="bibr" rid="scirp.35704-ref4">4</xref>], we use an algebraic method to find some of the salient features of the multispecies Calogero model on the line with twoand three-body interactions. After performing a certain transformation of the operator H, we get a new Hamiltonian <img src="2-1220051\2ed1929b-4ea4-4254-9dc0-422f6b14f7dd.jpg" /> for which we find its spectrum in the both cases with equal masses and different masses.</p></sec><sec id="s2"><title>2. Calogero Model with Different Masses</title><p>In this section, we reconsider the “multispecies” Calogero model considered in<img src="2-1220051\8de62d69-4ef0-4b05-bb04-4aeb9da5fd24.jpg" />. The Hamiltonian reads</p><disp-formula id="scirp.35704-formula50198"><label>(1)</label><graphic position="anchor" xlink:href="2-1220051\380eff42-2a53-4f4f-8972-ed50d7cc0312.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="2-1220051\97f115d8-07fb-4fa1-80aa-fcf59fc7c1b5.jpg" />.</p><p>We factorize the full ground state</p><disp-formula id="scirp.35704-formula50199"><label>(2)</label><graphic position="anchor" xlink:href="2-1220051\e04505f4-8dc8-44f3-a265-ec624c8468fb.jpg"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.35704-formula50200"><label>(3)</label><graphic position="anchor" xlink:href="2-1220051\0bfd1f61-c741-45b1-be37-439c6c0bbfd8.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50201"><label>(4)</label><graphic position="anchor" xlink:href="2-1220051\451194d6-7ddc-4dad-bbda-73a920a66299.jpg"  xlink:type="simple"/></disp-formula><p>When factorizing the factor <img src="2-1220051\28e91964-72b0-4e70-9f7e-67f72c7d9461.jpg" /> out of H, we got the new operator</p><disp-formula id="scirp.35704-formula50202"><label>(5)</label><graphic position="anchor" xlink:href="2-1220051\005d556c-64f9-4a07-a1ed-24448f13c87b.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50203"><label>(6)</label><graphic position="anchor" xlink:href="2-1220051\07a4ff79-a038-4f35-b3ed-030195a39b3a.jpg"  xlink:type="simple"/></disp-formula><p>The operator <img src="2-1220051\449efba1-7156-45c7-a121-d2eeee4fd5a1.jpg" /> preserves some spaces of polynomials that we would like to study and compare with the invariant spaces <img src="2-1220051\c5d5a748-bb85-4a2d-890a-4978ab9110ef.jpg" /> available in the case of equal masses, i.e. <img src="2-1220051\16d4ff9a-61a8-465e-b8f2-3af1a36e866e.jpg" />(the usual Calogero model). We first proceed with the <img src="2-1220051\e2558009-30b2-4d06-a7d2-14ebd2b3c9b2.jpg" /> i.e. two body case. Then it is easy to check that the following vector spaces are preserved by<img src="2-1220051\7b005648-c275-46f4-92de-d863b1a82b12.jpg" />:</p><disp-formula id="scirp.35704-formula50204"><label>(7)</label><graphic position="anchor" xlink:href="2-1220051\c8a871c6-ac65-4deb-9cd4-d1756ab596b2.jpg"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.35704-formula50205"><label>(8)</label><graphic position="anchor" xlink:href="2-1220051\e1fd4ea1-d0b5-4621-a74c-6bde50ae059c.jpg"  xlink:type="simple"/></disp-formula><p>It should be stressed that the combination <img src="2-1220051\6d6c288e-d60b-457a-85ce-830f6bedd76c.jpg" /> has to be eliminated from <img src="2-1220051\20435ee9-eb37-4606-bfd9-40fa12cd14dd.jpg" /> because it is not preserved by the part</p><disp-formula id="scirp.35704-formula50206"><label>(9)</label><graphic position="anchor" xlink:href="2-1220051\a27a610d-fba7-4cff-9bcc-c711ae344463.jpg"  xlink:type="simple"/></disp-formula><p>of the operator<img src="2-1220051\46191d65-320e-4428-ae5e-8caaea4d5664.jpg" />. As a consequence the monomial <img src="2-1220051\2225c7b6-6661-4e41-86ee-17c6ff650a86.jpg" /> has to be discarded from P<sub>3</sub> since <img src="2-1220051\29a2bad5-604c-42f5-92f6-2dc58d599390.jpg" /> i.e, the following part of the operator <img src="2-1220051\591fcad8-32ef-41c3-a188-655a7ca5d4b5.jpg" /></p><disp-formula id="scirp.35704-formula50207"><label>(10)</label><graphic position="anchor" xlink:href="2-1220051\c1f755f2-2e33-478a-8017-307ef3de4cff.jpg"  xlink:type="simple"/></disp-formula><p>would naturally involve a term of the form <img src="2-1220051\0a3a45b7-5596-449b-ab67-67052a495aed.jpg" /> in the first order monomial which is excluded by the above argument (i.e.<img src="2-1220051\d87a5c6f-e9e4-40e3-b184-7047eed15b54.jpg" />). Proceeding along the same lines we conclude that the set of spaces <img src="2-1220051\f8b06e1a-a046-4e2c-acf6-ae5903670a1f.jpg" /> can be rephased in terms of the vector spaces <img src="2-1220051\9e6fec8d-1030-4ef0-b5ed-d234b11d4391.jpg" /> defined in <img src="2-1220051\44bd0595-cdf2-4839-ba8a-cf24a5d591a5.jpg" /> i.e.</p><p><img src="2-1220051\47608a3e-9042-4cde-ac85-be2030f0adf1.jpg" /> <img src="2-1220051.files/image001.gif" /> (11)</p><p>with <img src="2-1220051\e8dbb19a-7439-481b-9171-a41efbdc911f.jpg" /> is the center-of-mass coordinate and &#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;<img src="2-1220051\d7214203-8520-4127-95e2-9baf2e4a4302.jpg" />&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160;&#160; (12)</p><p>in this respect, the operator H (and then also<img src="2-1220051\3be67f6b-aece-461a-a26e-002e26b9ed4b.jpg" />) is integrable and solvable for N = 2.</p><p>Notice that the space <img src="2-1220051\5e3246ee-b6c4-4125-b839-b9b453f885fd.jpg" /> is equivalent to the ones considered by [<xref ref-type="bibr" rid="scirp.35704-ref6">6</xref>], apart from the fact that the variable <img src="2-1220051\4cd6ddeb-4c6b-4bd0-ad87-a1a1a137ccec.jpg" /> (the analogue of<img src="2-1220051\94cb41d8-3317-491a-b6c8-93bc8ffa6702.jpg" />) is defined with the masses.</p><p>Let us now investigate the case N = 3. Again we can show that the following vector spaces are preserved by the operator<img src="2-1220051\9b5203d2-fa2b-4d05-9c81-eaef5189a56f.jpg" />,</p><disp-formula id="scirp.35704-formula50208"><label>(13)</label><graphic position="anchor" xlink:href="2-1220051\786fc1ee-045f-4dd6-bffd-76cfaee31a57.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.35704-formula50209"><label>(14)</label><graphic position="anchor" xlink:href="2-1220051\821d2916-20c5-4a16-990d-41f71ac973da.jpg"  xlink:type="simple"/></disp-formula><p>Note that <img src="2-1220051\f2684539-bb81-4e98-8f4e-c7b9c3bd0a12.jpg" /> above is the generalization of the variable <img src="2-1220051\29d5dd46-d321-4775-a22f-4e4c77144d99.jpg" /> of [<xref ref-type="bibr" rid="scirp.35704-ref6">6</xref>]. However, it turns out to be impossible to construct a translation invariant-cubic polynomial of the form</p><disp-formula id="scirp.35704-formula50210"><label>(15)</label><graphic position="anchor" xlink:href="2-1220051\32f04f61-0a7b-48a4-978a-891afa203e1b.jpg"  xlink:type="simple"/></disp-formula><p>which is preserved by the operator <img src="2-1220051\b270c7e0-e467-4461-9cf5-a3d9a8335805.jpg" /> if the masses m<sub>i</sub> are generic (i.e<img src="2-1220051\f38d78f1-be40-4bf0-beda-2c6c693146ff.jpg" />, etc). As a consequence, the dimension of the vector spaces of monomials preserved by <img src="2-1220051\b35e782e-73a8-4ed3-844a-676b4e2ba0b9.jpg" /> is lower than the vector spaces preserved by <img src="2-1220051\3f0c9827-f0bf-4ea1-ab4f-f0fec9968ac3.jpg" /> and the number of algebraic eigenvalues is lower than the usual Calogero case. In the next, this can be demonstrated easily in the particular case N = 2.</p><sec id="s2_1"><title>2.1. Eigenvalues for the Case with Equal Masses</title><p>We use the operator</p><disp-formula id="scirp.35704-formula50211"><label>(16)</label><graphic position="anchor" xlink:href="2-1220051\8ac864da-a9bd-4907-8cef-0c96def13b8f.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50212"><label>(17)</label><graphic position="anchor" xlink:href="2-1220051\c6b88fe6-261f-4fb5-b6e0-65c906cb433c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50213"><label>(18)</label><graphic position="anchor" xlink:href="2-1220051\e41ee70b-7d5d-4791-ad31-b3ad5e18a79a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50214"><label>(19)</label><graphic position="anchor" xlink:href="2-1220051\8ead0ace-911f-4431-9d8d-7c81c7567b03.jpg"  xlink:type="simple"/></disp-formula><p>The spectrum for the above case is 0;</p><p>1, 2;</p><p>2, 3, 4.</p></sec><sec id="s2_2"><title>2.2. Eigenvalues for the Case with Different Masses</title><p>In this case we apply the some procedure used in the previous case (i.e. we consider also N = 2) but the operator D has the following form</p><disp-formula id="scirp.35704-formula50215"><label>(20)</label><graphic position="anchor" xlink:href="2-1220051\fb618d3c-e2f9-47bc-8012-6d49a27c88dc.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50216"><label>(21)</label><graphic position="anchor" xlink:href="2-1220051\7a491e68-92bf-4c21-8362-107f4b6be9b9.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50217"><label>(22)</label><graphic position="anchor" xlink:href="2-1220051\204f99d7-0b31-4bd1-b617-4b5329fc16e1.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.35704-formula50218"><label>(23)</label><graphic position="anchor" xlink:href="2-1220051\5530017e-5533-44ae-b280-62e3d95fa9ed.jpg"  xlink:type="simple"/></disp-formula><p>The spectrum for the above case is 0;</p><p>1;</p><p>2, 2.</p><p>More generally, the vector spaces preserved by <img src="2-1220051\99cebc96-cad1-4295-9f7b-bc3c7a041f9c.jpg" /> are of the form</p><disp-formula id="scirp.35704-formula50219"><label>(24)</label><graphic position="anchor" xlink:href="2-1220051\ac7d1e87-d983-4752-9005-12417a44551c.jpg"  xlink:type="simple"/></disp-formula><p>and any eigenvector of <img src="2-1220051\52338293-819e-45e8-b7ff-7f0f16b12560.jpg" /> can be written according to</p><disp-formula id="scirp.35704-formula50220"><label>(25)</label><graphic position="anchor" xlink:href="2-1220051\8f3458c5-2b7e-44da-9295-e25a5dc61491.jpg"  xlink:type="simple"/></disp-formula><p>while the corresponding eigenvalues are given by</p><disp-formula id="scirp.35704-formula50221"><label>(26)</label><graphic position="anchor" xlink:href="2-1220051\99d93a62-08f1-4b72-a4f9-dd603c7c0468.jpg"  xlink:type="simple"/></disp-formula><p>so that the spectrum of <img src="2-1220051\0a672c87-87a0-42de-a3ab-1dc07cce5bd9.jpg" /> consists of integers of the form</p><disp-formula id="scirp.35704-formula50222"><label>(27)</label><graphic position="anchor" xlink:href="2-1220051\d5763bc9-64b3-47d0-b12e-80004788bca1.jpg"  xlink:type="simple"/></disp-formula><p>as generic in [<xref ref-type="bibr" rid="scirp.35704-ref5">5</xref>]. In this way, we have redemonstrated the result of these authors by following the algebraic technique of operators preserving spaces of monomials as suggested by [<xref ref-type="bibr" rid="scirp.35704-ref6">6</xref>].</p><p>We have attempted to construct invariant spaces of polynomials involving the monomials</p><disp-formula id="scirp.35704-formula50223"><label>(28)</label><graphic position="anchor" xlink:href="2-1220051\406bedf3-f88d-4ba7-9986-1d0da65b3f5d.jpg"  xlink:type="simple"/></disp-formula><p>with<img src="2-1220051\f7e319c3-31e7-44bd-b7cc-4347ffbae85f.jpg" />. These polynomials are indeed such that <img src="2-1220051\12607e0a-8360-486f-82e6-7eb7e2f792f4.jpg" /> is a polynomial but the new polynomials <img src="2-1220051\faf4885b-9bb8-47cc-9a66-141c02d8d86c.jpg" /> are not in general expressible as polynomials of the two variables X and <img src="2-1220051\29894c5a-3891-4ddf-9c39-81aae9b6ecb2.jpg" /> (i.e.<img src="2-1220051\abb3a7bf-d606-440b-93ce-c672334c3acf.jpg" />). More generally, the polynomials for <img src="2-1220051\9d60b77c-1585-4b7e-99c0-785399949af0.jpg" /> body can be written as follows</p><disp-formula id="scirp.35704-formula50224"><label>(29)</label><graphic position="anchor" xlink:href="2-1220051\a0b60237-ea90-4bca-87ca-f3c0bee7bf60.jpg"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s3"><title>3. Conclusion</title><p>Here we have constructed the operator <img src="2-1220051\3aed0779-7586-4b05-a45a-f1145eedca75.jpg" /> which preserves some spaces of polynomials and compared with the invariant spaces available in the usual Calogero model (<img src="2-1220051\c142eb5b-d104-470a-ac41-99e005b7c0af.jpg" />i.e. the masses are equal). We have determined the real spectrum for the case with different masses and for the case for equal masses where <img src="2-1220051\6ff244fd-53d0-4f75-b5eb-52efba457b76.jpg" /> i.e. two body case. This extended Calogero model exhibits some remarkable properties which are absent in the case of usual Calogero model. For example, the number of eigenvalues in the case with different masses is lower than one of eigenvalues of the usual Calogero model.</p></sec><sec id="s4"><title>4. Acknowledgements</title><p>I thank Pr. Yves Brihaye for useful discussions</p></sec><sec id="s5"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.35704-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">F. Calogero, “Solution of a Three-Body Problem in One Dimension,” Journal of Mathematical Physics, Vol. 10, No. 12, 1969, pp. 2191-2197. doi:10.1063/1.1664820</mixed-citation></ref><ref id="scirp.35704-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">F. 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