<?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>S0035-001X2010000200011</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Anisotropic cosmology in Sáez-Ballester theory: classical and quantum solutions]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Socorro]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sabido]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sánchez]]></surname>
<given-names><![CDATA[M.A.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Frías Palos]]></surname>
<given-names><![CDATA[M.G.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad de Guanajuato Departamento de Física Campus León]]></institution>
<addr-line><![CDATA[Guanajuato ]]></addr-line>
<country>México</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad Autónoma del Estado de México Facultad de Ciencias ]]></institution>
<addr-line><![CDATA[Toluca Edo de Mex]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>04</month>
<year>2010</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>04</month>
<year>2010</year>
</pub-date>
<volume>56</volume>
<numero>2</numero>
<fpage>166</fpage>
<lpage>171</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2010000200011&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2010000200011&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2010000200011&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[We use the Sáez-Ballester theory on anisotropic Bianchi I cosmological model, with barotropic flui and cosmological constant. We obtain the classical solution by using the Hamilton-Jacobi approach. Also the quantum regime is constructed and exact solutions to the Wheeler-DeWitt equation are found.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Usamos la teoría de Sáez-Ballester en el modelo anisotrópico Bianchi I con un fluid barotrópico y constante cosmológica. Obtenemos las soluciones clásicas usando el enfoque de Hamilton-Jacobi. El regimen cuántico también es construido y soluciones exactas a la ecuación de Wheeler-DeWitt son encontradas.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Classical and quantum exact solutions]]></kwd>
<kwd lng="en"><![CDATA[cosmology]]></kwd>
<kwd lng="es"><![CDATA[Soluciones clásicas y cuánticas exactas]]></kwd>
<kwd lng="es"><![CDATA[cosmología]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Investigaci&oacute;n</font></p>     <p align="justify"><font face="verdana" size="4">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Anisotropic cosmology in S&aacute;ez&#150;Ballester theory: classical and quantum solutions</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>J. Socorro<sup>1*</sup>, M. Sabido<sup>1**</sup>, M.A. S&aacute;nchez<sup>2</sup> and M.G. Fr&iacute;as Palos<sup>2</sup></b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i><sup>1</sup> Departamento de F&iacute;sica, DCel, Universidad de Guanajuato&#150;Campus Le&oacute;n, Apartado Postal E&#150;143, 37150, Guanajuato, M&eacute;xico. E&#150;mail: </i>*<a href="mailto:socorro@fisica.ugto.m">socorro@fisica.ugto.m</a><i>; </i>**<a href="mailto:msabido@fisica.ugto.m">msabido@fisica.ugto.m</a></font></p>     <p align="justify"><font face="verdana" size="2"><i><sup>2</sup> Facultad de Ciencias de la Universidad Aut&oacute;noma del Estado de M&eacute;xico, Instituto Literario No. 100, Toluca, 50000, Edo de Mex, M&eacute;xico.</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 25 de noviembre de 2009    ]]></body>
<body><![CDATA[<br> Aceptado el 16 de marzo de 2010</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">We use the S&aacute;ez&#150;Ballester theory on anisotropic Bianchi I cosmological model, with barotropic flui and cosmological constant. We obtain the classical solution by using the Hamilton&#150;Jacobi approach. Also the quantum regime is constructed and exact solutions to the Wheeler&#150;DeWitt equation are found.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Classical and quantum exact solutions; cosmology.</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">Usamos la teor&iacute;a de S&aacute;ez&#150;Ballester en el modelo anisotr&oacute;pico Bianchi I con un fluid barotr&oacute;pico y constante cosmol&oacute;gica. Obtenemos las soluciones cl&aacute;sicas usando el enfoque de Hamilton&#150;Jacobi. El regimen cu&aacute;ntico tambi&eacute;n es construido y soluciones exactas a la ecuaci&oacute;n de Wheeler&#150;DeWitt son encontradas.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores: </b>Soluciones cl&aacute;sicas y cu&aacute;nticas exactas; cosmolog&iacute;a. </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: 02.30.Jr; 04.60.Kz; 12.60Jv; 98.80.Qc.</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/v56n2/v56n2a11.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>Acknowledgments</b></font></p>     <p align="justify"><font face="verdana" size="2">This work was partially supported by CONACYT grants 51306, 56946 and 62253. DINPO (2009) and PROMEP grants UGTO&#150;CA&#150;3 and UGTO&#150;PTC&#150;085. This work is part of the collaboration within the Instituto Avanzado de Cosmolog&iacute;a. Many calculations where done by Symbolic Program REDUCE 3.8.</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. D. Saez and V.J. Ballester, <i>Phys. Lett. A </i><b>113 </b>(1986) 467.</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=8359216&pid=S0035-001X201000020001100001&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. T. Singh and A.K. Agrawal, <i>Astrophys. 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