<?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>S0035-001X2014000100014</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Black holes from Myers-Perry solution]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[López]]></surname>
<given-names><![CDATA[L. A.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Autónoma del Estado de Hidalgo Área Académica de Matemáticas y Física ]]></institution>
<addr-line><![CDATA[Pachuca Hidalgo]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>02</month>
<year>2014</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>02</month>
<year>2014</year>
</pub-date>
<volume>60</volume>
<numero>1</numero>
<fpage>95</fpage>
<lpage>101</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2014000100014&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2014000100014&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2014000100014&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[From the five dimensional Myers-Perry solution and consider that de metric MP corresponding to the Kaluza-Klein ansatz (zero mode), we obtained 4D solution with non-minimally coupled scalar and electromagnetic fields, characterized by three parameters, r0 , a, b, related to the mass, angular momentum and electromagnetic field, respectively and proposing that the 4D solution is a solution type black hole. Then for a &#8800; 0, b = 0 the electromagnetic field vanishes and the black hole is stationary. For a = 0, b &#8800; 0 the solution is static with electric field. If a &#8800; 0, b &#8800; 0 the solution is stationary with electric field and, due to the rotation, a magnetic field appears. The scalar field that arises from the dimensional reduction is present in all cases. At infinity the solution is asymptotically flat and the trace of the scalar field get lost, turning out that this solution is in agreement with the no hair conjecture.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Exact solutions]]></kwd>
<kwd lng="en"><![CDATA[higher dimensions]]></kwd>
<kwd lng="en"><![CDATA[black holes]]></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="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="4"><b>Black holes from Myers&#45;Perry solution</b></font></p>  	    <p align="center"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="2"><b>L. A. L&oacute;pez</b></font></p>  	    <p align="center"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><i>&Aacute;rea Acad&eacute;mica de Matem&aacute;ticas y F&iacute;sica, UAEH, carretera Pachuca&#45;Tulancingo km 4.5, Pachuca, 42184, Hidalgo, 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">Received 5 August 2013<i>.</i>    ]]></body>
<body><![CDATA[<br> 	Accepted 15 November 2013<i>.</i></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">From the five dimensional Myers&#45;Perry solution and consider that de metric MP corresponding to the Kaluza&#45;Klein ansatz (zero mode), we obtained 4D solution with non&#45;minimally coupled scalar and electromagnetic fields, characterized by three parameters, <i>r<sub>0</sub> , a, b,</i> related to the mass, angular momentum and electromagnetic field, respectively and proposing that the 4D solution is a solution type black hole. Then for <i>a</i> &#8800; 0, <i>b</i> = 0 the electromagnetic field vanishes and the black hole is stationary. For <i>a</i> = 0, <i>b</i> &#8800; 0 the solution is static with electric field. If <i>a</i> &#8800; 0, <i>b</i> &#8800; <i>0</i> the solution is stationary with electric field and, due to the rotation, a magnetic field appears. The scalar field that arises from the dimensional reduction is present in all cases. At infinity the solution is asymptotically flat and the trace of the scalar field get lost, turning out that this solution is in agreement with the no hair conjecture.</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>Keywords:</b> Exact solutions; higher dimensions; black holes.</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2">PACS: 04.70.Bw; 04.50.Gh; 04.50.Cd; 04.20.Jb</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/v60n1/v60n1a14.pdf" target="_blank">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    ]]></body>
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