<?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>0035-001X</journal-id>
<journal-title><![CDATA[Revista mexicana de física]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fis.]]></abbrev-journal-title>
<issn>0035-001X</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0035-001X2006000900032</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Soluciones conformemente planas con ecuación de estado no local]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Muñoz S]]></surname>
<given-names><![CDATA[A. G]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Núñez]]></surname>
<given-names><![CDATA[L. A]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad del Zulia Facultad de Ciencias Departamento de Física]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>Venezuela</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad de Los Andes Facultad de Ciencias Centro Nacional de Cálculo Científico]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>Venezuela</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<volume>52</volume>
<fpage>112</fpage>
<lpage>115</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2006000900032&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2006000900032&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2006000900032&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Una ecuación de estado no local describe las componentes del tensor de energía-impulso no sólo como función de un punto, sino como un funcional que toma en consideración la contribución de toda la configuración de materia encerrada hasta ese punto. En este trabajo se muestra que es posible obtener distribuciones de materia físicamente aceptables que poseen simultaneamente tanto una métrica conformemente plana como una ecuación de estado no local. Se presenta la evolución de objetos compactos en distintos escenarios, determinando para el caso cuasi-estático las condiciones para la aparición de exfoliación térmica.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[A non-local equation of state describes the components of the energy-momentum tensor not only as a function of a point, but as a functional throughout the enclosed configuration. In this work, we show that it is possible to obtain physically acceptable conformally flat, anisotropic matter distributions that satisfy a non-local equation of state. The evolution of such objects is presented, determining for the quasi-static case the conditions for thermic-peeling effect.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[Ecuación de estado no-local]]></kwd>
<kwd lng="es"><![CDATA[fluidos anisótropos relativistas]]></kwd>
<kwd lng="es"><![CDATA[métricas conformemente planas]]></kwd>
<kwd lng="es"><![CDATA[exfoliación térmica]]></kwd>
<kwd lng="en"><![CDATA[Non-local equation of state]]></kwd>
<kwd lng="en"><![CDATA[relativistic anisotropic matter distributions]]></kwd>
<kwd lng="en"><![CDATA[conformally flat metrics]]></kwd>
<kwd lng="en"><![CDATA[thermic peeling]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">F&iacute;sica Te&oacute;rica </font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Soluciones conformemente planas con ecuaci&oacute;n de estado no local</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>A.G. Mu&ntilde;oz S.* y L.A. N&uacute;&ntilde;ez**</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>* Grupo de Investigaciones de F&iacute;sica Te&oacute;rica (GIFT) Departamento de F&iacute;sica, Facultad de Ciencias, La Universidad del Zulia, Maracaibo 4004, Venezuela, Postgrado en F&iacute;sica Fundamental, Centro de Astrof&iacute;sica Te&oacute;rica (CAT), Facultad de Ciencias, Universidad de Los Andes, M&eacute;rida, 5101, Venezuela e&#150;mail: <a href="mailto:agmunoz@luz.edu.ve">agmunoz@luz.edu.ve</a></i></font></p>     <p align="justify"><font face="verdana" size="2"><i>** Centro de Astrof&iacute;sica Te&oacute;rica (CAT), Facultad de Ciencias, Universidad de Los Andes, M&eacute;rida 5101, Venezuela, Centro Nacional de C&aacute;lculo Cient&iacute;fico Universidad de Los Andes (CeCalCULA), Corporaci&oacute;n Parque Tecnol&oacute;gico de M&eacute;rida, M&eacute;rida 5101, Venezuela, e&#150;mail: <a href="mailto:nunez@ula.ve">nunez@ula.ve</a></i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 4 de noviembre de 2003    ]]></body>
<body><![CDATA[<br>   Aceptado el 19 de junio de 2004</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">Una ecuaci&oacute;n de estado no local describe las componentes del tensor de energ&iacute;a&#150;impulso no s&oacute;lo como funci&oacute;n de un punto, sino como un funcional que toma en consideraci&oacute;n la contribuci&oacute;n de toda la configuraci&oacute;n de materia encerrada hasta ese punto. En este trabajo se muestra que es posible obtener distribuciones de materia f&iacute;sicamente aceptables que poseen simultaneamente tanto una m&eacute;trica conformemente plana como una ecuaci&oacute;n de estado no local. Se presenta la evoluci&oacute;n de objetos compactos en distintos escenarios, determinando para el caso cuasi&#150;est&aacute;tico las condiciones para la aparici&oacute;n de exfoliaci&oacute;n t&eacute;rmica.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> Ecuaci&oacute;n de estado no&#150;local; fluidos anis&oacute;tropos relativistas; m&eacute;tricas conformemente planas; exfoliaci&oacute;n t&eacute;rmica.</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">A non&#150;local equation of state describes the components of the energy&#150;momentum tensor not only as a function of a point, but as a functional throughout the enclosed configuration. In this work, we show that it is possible to obtain physically acceptable conformally flat, anisotropic matter distributions that satisfy a non&#150;local equation of state. The evolution of such objects is presented, determining for the quasi&#150;static case the conditions for thermic&#150;peeling effect.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Non&#150;local equation of state; relativistic anisotropic matter distributions; conformally flat metrics; thermic peeling.</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: 04.20.Ex; 04.20.Jb; 04.40.Dg</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmf/v52s3/v52s3a32.pdf">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>Referencias</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. N.K. Glendenning, <i>Compact Stars </i>(New York: Springer Verlag,&nbsp;2000).</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=8379804&pid=S0035-001X200600090003200001&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. L. Herrera, A. Di Prisco, J. Ospino y E. Fuenmayor, <i>J. Math. Phys. </i><b>42</b> (2001) 2129 (tambi&eacute;n en e&#150;print, gr&#150;qc/0102058).</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=8379805&pid=S0035-001X200600090003200002&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. L. Herrera y N.O. Santos, <i>Gen. Rel. Grav. </i><b>27</b> (1995) 1071.&nbsp;</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=8379806&pid=S0035-001X200600090003200003&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. H. Hern&aacute;ndez, L. N&uacute;&ntilde;ez y U. Percoco, <i>Class. Quantum Grav.</i>&nbsp;<b>16</b> (1999) 897.&nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp; &nbsp;</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=8379807&pid=S0035-001X200600090003200004&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. R. Kippenhahn y A. Weigert, <i>Stellar Structure and Evolution</i> (Berlin: Springer Verlag, 1990).</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=8379808&pid=S0035-001X200600090003200005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
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</article>
