<?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>2304-0106</journal-id>
<journal-title><![CDATA[Anales de la Academia de Ciencias de Cuba]]></journal-title>
<abbrev-journal-title><![CDATA[Anales de la ACC]]></abbrev-journal-title>
<issn>2304-0106</issn>
<publisher>
<publisher-name><![CDATA[Academia de Ciencias de Cuba]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S2304-01062022000300014</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Modelación de objetos compactos anisotrópicos]]></article-title>
<article-title xml:lang="en"><![CDATA[Theoretical modeling of anisotropic compact objects]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[P´erez Mart´&#305;nez]]></surname>
<given-names><![CDATA[Aurora]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Quintero Angulo]]></surname>
<given-names><![CDATA[Gretel]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Alvear Terrero]]></surname>
<given-names><![CDATA[Diana]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Pérez Rojas]]></surname>
<given-names><![CDATA[Hugo]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Manreza Paret]]></surname>
<given-names><![CDATA[Daryel]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Suárez González]]></surname>
<given-names><![CDATA[Lismary de la Caridad]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[López Pérez]]></surname>
<given-names><![CDATA[Samantha]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Instituto de Cibern´etica Matem´atica y F´&#305;sica (ICIMAF)  ]]></institution>
<addr-line><![CDATA[ La Habana]]></addr-line>
<country>Cuba</country>
</aff>
<aff id="Af2">
<institution><![CDATA[,Universidad de La Habana Facultad de F´&#305;sica ]]></institution>
<addr-line><![CDATA[ La Habana]]></addr-line>
<country>Cuba</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>12</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>12</month>
<year>2022</year>
</pub-date>
<volume>12</volume>
<numero>3</numero>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_arttext&amp;pid=S2304-01062022000300014&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_abstract&amp;pid=S2304-01062022000300014&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.sld.cu/scielo.php?script=sci_pdf&amp;pid=S2304-01062022000300014&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[RESUMEN  Introducción.  La comprensión de la composición y la estructura macroscópica de los Objetos Compactos constituye uno de los mayores desafíos de la Astrofísica. En particular, si estos están magnetizados, pues en este caso nos encontramos ante el problema, aún no resuelto, de hallar la estructura de una estrella cuya forma no es esférica.  Métodos.  Dando continuidad a nuestros estudios dentro de esta temática, en el presente trabajo se construyen, a partir de las Ecuaciones de Einstein, un sistema de ecuaciones de estructura aproximadas para objetos compactos esferoidales. Dichas ecuaciones tienen un carácter general y han sido utilizadas exitosamente para el estudio de Enanas Blancas, Estrellas de condensado de Bose-Einstein y Estrellas Extrañas magnetizadas.  Resultado.  En paralelo, se obtuvieron soluciones de las ecuaciones de Einstein aplicables a la descripción de las magnetosferas estelares, y se realizó un estudio preliminar de un modelo de jets astrofísicos.  Conclusiones.  A partir de estas investigaciones fue posible demostrar que un campo magnético uniforme no incrementa la masa máxima de estas estrellas, siendo su mayor efecto contribuir a la deformación de los mismas. Asimismo, se propuso y validó un mecanismo para la generación del campo magnético, lo cual constituye una de las mayores novedades del trabajo, y se comprobó que son las estrellas de masas intermedias las que causarían las ondas gravitacionales de mayor amplitud.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[ABSTRACT  Introduction. The understanding of the composition and macroscopic properties of compact objects is one of the biggest challenges of Astrophysics. In particular, if the object is magnetized, one faces the still unsolved problem of finding the structure of a non-spherical star. Following our studies on these topics, here we present a set of structure equations for spheroidal compact objects, as long as they are not too far from the spherical shape.  Methods. These equations describe any compact object whose equation of state has magnetic anisotropy, and have been successfully applied to the study of magnetized White Dwarfs, Bose-Einstein condensate Stars and Strange Stars.  Results and Discussion.  As collateral results, we obtained solutions to Einstein&#8217;s equations suitable for describing the magnetosphere of compact objects, and performed a preliminary study of a model for astrophysical jets.  Conclusions.  From these studies, we show that a uniform magnetic field does not increase the maximum mass of compact objects, its biggest effect being their deformation. In addition, we proposed and validated a mechanism for the generation of the stellar magnetic field, which constitutes one of the major novelties of the work, and found that the stars of intermediate masses are the candidates to produce the most intense gravitational waves.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[objetos compactos magnetizados]]></kwd>
<kwd lng="es"><![CDATA[enanas blancas]]></kwd>
<kwd lng="es"><![CDATA[estrellas de neutrones]]></kwd>
<kwd lng="es"><![CDATA[espacio-tiempo axisimétrico]]></kwd>
<kwd lng="en"><![CDATA[magnetized compact objects]]></kwd>
<kwd lng="en"><![CDATA[white dwarfs]]></kwd>
<kwd lng="en"><![CDATA[neutron stars: axisymmetric spacetimes]]></kwd>
</kwd-group>
</article-meta>
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