<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1870-3542</journal-id>
<journal-title><![CDATA[Revista mexicana de física E]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fís. E]]></abbrev-journal-title>
<issn>1870-3542</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1870-35422007000100010</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[The exactly solvable self-gravitating fermion cluster in two dimensions]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sañudo]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Pacheco]]></surname>
<given-names><![CDATA[A.F.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad de Extremadura Departamento de Física ]]></institution>
<addr-line><![CDATA[Badajoz ]]></addr-line>
<country>Spain</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad de Zaragoza Facultad de Ciencias Biocomputación y Física de Sistemas Complejos (BIFI)]]></institution>
<addr-line><![CDATA[Zaragoza ]]></addr-line>
<country>Spain</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2007</year>
</pub-date>
<volume>53</volume>
<numero>1</numero>
<fpage>82</fpage>
<lpage>85</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S1870-35422007000100010&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S1870-35422007000100010&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S1870-35422007000100010&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[The mathematical model of a two-dimensional self-gravitating cluster formed by degenerate fermions, is solved analytically. The fermions interact with each other through a logarithmic potential. The radius of this system is shown to be constant, not depending on the total number of fermions that constitute the cluster.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[En este artículo resolvemos analíticamente el modelo matemático de un cúmulo autogravitante de fermiones degenerados, en dos dimensiones. Los fermiones interactúan entre ellos mediante un potencial logarítmico. El radio resultante para el cúmulo no depende del número total de fermiones que lo integran.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Thomas-Fermi model]]></kwd>
<kwd lng="en"><![CDATA[white dwarfs]]></kwd>
<kwd lng="es"><![CDATA[Modelo de Thomas Fermi]]></kwd>
<kwd lng="es"><![CDATA[enana blanca]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Ense&ntilde;anza</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>The exactly solvable self&#150;gravitating fermion cluster in two dimensions</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>J. Sa&ntilde;udo&ordf; and A.F. Pacheco<sup>b</sup></b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">&ordf;<i> Departamento de F&iacute;sica, Universidad de Extremadura, 06071 Badajoz, Spain, Tel: 34924289525, FAX: 34924289651, </i>e&#150;mail: <a href="mailto:jsr@unex.es">jsr@unex.es</a></font></p>     <p align="justify"><font face="verdana" size="2"> <sup>b</sup><i> Facultad de Ciencias and BIFI, Universidad de Zaragoza, 50009 Zaragoza, Spain, Tel: 34976761135, FAX: 34976761140, </i>e&#150;mail: <a href="mailto:amalio@unizar.es">amalio@unizar.es</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 23 de junio de 2006    ]]></body>
<body><![CDATA[<br> Aceptado el 9 de agosto de 2006</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Abstract</b></font></p>     <p align="justify"><font face="verdana" size="2">The mathematical model of a two&#150;dimensional self&#150;gravitating cluster formed by degenerate fermions, is solved analytically. The fermions interact with each other through a logarithmic potential. The radius of this system is shown to be constant, not depending on the total number of fermions that constitute the cluster.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Thomas&#150;Fermi model; white dwarfs.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Resumen</b></font></p>     <p align="justify"><font face="verdana" size="2">En este art&iacute;culo resolvemos anal&iacute;ticamente el modelo matem&aacute;tico de un c&uacute;mulo autogravitante de fermiones degenerados, en dos dimensiones. Los fermiones interact&uacute;an entre ellos mediante un potencial logar&iacute;tmico. El radio resultante para el c&uacute;mulo no depende del n&uacute;mero total de fermiones que lo integran.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores: </b>Modelo de Thomas Fermi; enana blanca. </font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">PACS: 31.5.Bs; 97.20.Rp</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmfe/v53n1/v53n1a10.pdf" target="_blank">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Acknowledgements</b></font></p>     <p align="justify"><font face="verdana" size="2">This work was supported in part by the Spanish DGICYT under Project FIS2005&#150;06237.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. See, for example, S.L. Shapiro, and S.A. Teukolsky, <i>Black Holes,  White Dwarfs, and Neutron Stars </i>(New York:  Wiley, 1983).</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446612&pid=S1870-3542200700010001000001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">2. See, for example, S. Eliezer, A. Ghatak, and H. Hora, <i>An Introduction to Equations of State </i>(Cambridge: Cambridge U.P., 1986).</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446613&pid=S1870-3542200700010001000002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">3. R.K. Bhaduri, S. Das Gupta, and S.L. Lee, <i>Am. J. Phys. </i><b>58</b> (1990) 983.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446614&pid=S1870-3542200700010001000003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">4. G.F. Kventsel and J. Katriel, <i>Phys. Rev. A </i><b>24 </b>(1981) 2299.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446615&pid=S1870-3542200700010001000004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">5. J. Ostriker, <i>Ap. J. </i><b>140 </b>(1964) 1056.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446616&pid=S1870-3542200700010001000005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">6. See, for example, M. Abramowitz and I.A. Stegun (Editors) <i>Handbook of Mathematical Functions </i>(New York: Dover Publications, 1970)</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446617&pid=S1870-3542200700010001000006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">7. R. Pino, <i>Phys. Rev. B </i><b>58</b> (1998) 4644.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446618&pid=S1870-3542200700010001000007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --><p align="justify"><font face="verdana" size="2">8. M. Membrado, A.F. Pacheco, and J. Sa&ntilde;udo, <i>Astron. Astrophys. </i><b>217 </b>(1989) 92.</font>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8446619&pid=S1870-3542200700010001000008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
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