<?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>S0035-001X2022000500010</article-id>
<article-id pub-id-type="doi">10.31349/revmexfis.68.050704</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Modos cuasi-normales de un agujero negro de Einstein-Gauss-Bonnet rodeado de quintaesencia: perturbaciones escalares y electromagnéticas]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Barrientos]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Pedraza]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[López]]></surname>
<given-names><![CDATA[L. A.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Arceo]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,UAEH Area Académica de Matemáticas y Física ]]></institution>
<addr-line><![CDATA[ Hidalgo]]></addr-line>
<country>Mexico</country>
</aff>
<aff id="Af2">
<institution><![CDATA[,Universidad Autónoma de Chiapas Facultad de Ciencias en Física y Matemáticas ]]></institution>
<addr-line><![CDATA[Tuxtla Gutiérrez Chiapas]]></addr-line>
<country>Mexico</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>10</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>10</month>
<year>2022</year>
</pub-date>
<volume>68</volume>
<numero>5</numero>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2022000500010&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2022000500010&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2022000500010&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen En este trabajo, se estudian los modos cuasi-normales para perturbaciones escalares y electromagnéticas en un agujero negro de Einstein-Gauss-Bonnet rodeado de quintaesencia empleando el método WKB a tercer orden y el límite Eikonal. Primeramente, se establecen los valores críticos de la constante de acoplamiento de Gauss-Bonnet y del factor de normalización relacionado con la quintaesencia, con el fin de describir los horizontes de eventos de la solución. El estudio de la condición de horizontes extremos y los modos cuasi-normales es realizado estableciendo el parámetro de estado de quintaesencia en el caso particular de &#969;q = -2/3.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract In this work, we study the quasi-normal modes for scalar and electromagnetic perturbations for an Einstein-Gauss-Bonnet black hole surrounded by quintessence using the third-order WKB method and the Eikonal limit. First, the critical values of the Gauss-Bonnet coupling constant and the normalization factor related to the quintessence are established, to describe the event horizons of the solution. We have studied the condition of extreme horizons and the quasi-normal modes are performed by setting the quintessence state parameter in the particular case of &#969;q = -2/3.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[cuasi-normales]]></kwd>
<kwd lng="es"><![CDATA[quintaesencia]]></kwd>
<kwd lng="es"><![CDATA[aproximación WKB]]></kwd>
<kwd lng="es"><![CDATA[exponente de Lyapunov]]></kwd>
<kwd lng="en"><![CDATA[Quasi-normal modes]]></kwd>
<kwd lng="en"><![CDATA[quintessence, WKB approximation]]></kwd>
<kwd lng="en"><![CDATA[Lyapunov exponent]]></kwd>
</kwd-group>
</article-meta>
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