<?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>S0035-001X2014000300003</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Retardo temporal en las lentes por galaxias en el contexto de Reissner - Nordstrom]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Miranda]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Molina]]></surname>
<given-names><![CDATA[U.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Viloria]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
<xref ref-type="aff" rid="A03"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad de Sucre Departamento de física ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad del Atlántico Departamento de física ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<aff id="A03">
<institution><![CDATA[,Universidad de la Costa CUC Departamento de Ciencias Básicas ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2014</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2014</year>
</pub-date>
<volume>60</volume>
<numero>3</numero>
<fpage>190</fpage>
<lpage>194</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2014000300003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2014000300003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2014000300003&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[En este trabajo se deducen las expresiones matemáticas para el retardo temporal entre dos imágenes debidas a una lente gravitacional con distribuciones simétricas tanto de masa como de carga eléctrica a partir del elemento de línea en el contexto de Reissner - Nordstrom (RN). Para esto, se estudia el movimiento de fotones que se curvan cerca de la distribución de masa cargada, mediante la métrica de RN, obteniendo las expresiones para el ángulo de desviación y el potencial de deflexión, estudiando así el fenómeno de lentes gravitacionales tanto para una masa puntual como para una distribución de masa. Luego se aplican los resultados obtenidos, al modelo de la esfera singular isoterma (ESI), y se comparan con aquellos en los cuales técnicamente se considera galaxias con distribución de masa. Pero, cabe destacar que esta expresión del retardo temporal es aplicable a cualquier modelo de lente gravitacional cargado.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[In this work we derive the mathematical expressions for the time delay between two images due to gravitational lensing with symmetric distributions of both: mass and electric charge from the line element in the context of Reissner - Nordstrom (RN). For this, is important to study the motion of photons that are curved around the mass distribution charged by RN metric, obtaining expressions for the deflection angle and deflection potential studying the phenomenon of so much for a lensing precise mass to mass distribution. Then applied the results, the singular sphere model isotherm (ESI), and compared with those in which only considers galaxies mass distribution. But, that this expression of the time delay is applicable to any gravitational lens model loaded too.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[Retardo temporal]]></kwd>
<kwd lng="es"><![CDATA[lentes gravitacionales con carga eléctrica]]></kwd>
<kwd lng="en"><![CDATA[Time delay]]></kwd>
<kwd lng="en"><![CDATA[electrically charged gravitational lenses]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[  	    <p align="justify"><font face="verdana" size="4">Research</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="4"><b>Retardo temporal en las lentes por galaxias en el contexto de Reissner &#45; Nordstrom</b></font></p>  	    <p align="center"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="2"><b>C. Miranda<sup>a</sup>, U. Molina<sup>b</sup> y P. Viloria<sup>c</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>a</sup></i> <i>Departamento de f&iacute;sica, Universidad de Sucre.</i></font></p>  	    <p align="justify"><font face="verdana" size="2"><i><sup>b</sup> Departamento de f&iacute;sica, Universidad del Atl&aacute;ntico.</i></font></p>  	    <p align="justify"><font face="verdana" size="2"><i><sup>c</sup> Departamento de Ciencias B&aacute;sicas, Universidad de la Costa CUC.</i></font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2">Received 6 January 2014    <br> 	accepted 7 March 2014</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 trabajo se deducen las expresiones matem&aacute;ticas para el retardo temporal entre dos im&aacute;genes debidas a una lente gravitacional con distribuciones sim&eacute;tricas tanto de masa como de carga el&eacute;ctrica a partir del elemento de l&iacute;nea en el contexto de Reissner &#45; Nordstrom (RN). Para esto, se estudia el movimiento de fotones que se curvan cerca de la distribuci&oacute;n de masa cargada, mediante la m&eacute;trica de RN, obteniendo las expresiones para el &aacute;ngulo de desviaci&oacute;n y el potencial de deflexi&oacute;n, estudiando as&iacute; el fen&oacute;meno de lentes gravitacionales tanto para una masa puntual como para una distribuci&oacute;n de masa. Luego se aplican los resultados obtenidos, al modelo de la esfera singular isoterma (ESI), y se comparan con aquellos en los cuales t&eacute;cnicamente se considera galaxias con distribuci&oacute;n de masa. Pero, cabe destacar que esta expresi&oacute;n del retardo temporal es aplicable a cualquier modelo de lente gravitacional cargado.</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> Retardo temporal; lentes gravitacionales con carga el&eacute;ctrica.</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">In this work we derive the mathematical expressions for the time delay between two images due to gravitational lensing with symmetric distributions of both: mass and electric charge from the line element in the context of Reissner &#45; Nordstrom (RN). For this, is important to study the motion of photons that are curved around the mass distribution charged by RN metric, obtaining expressions for the deflection angle and deflection potential studying the phenomenon of so much for a lensing precise mass to mass distribution. Then applied the results, the singular sphere model isotherm (ESI), and compared with those in which only considers galaxies mass distribution. But, that this expression of the time delay is applicable to any gravitational lens model loaded too.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2"><b>Keywords:</b> Time delay; electrically charged gravitational lenses.</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2">PACS: 95.30.Sf; 98.62.Sb; 98.80.Es; 98.62.Py</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/v60n3/v60n3a3.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>Referencias</b></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">1.&nbsp;R. Adler, M. Schiffer, y J. 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