<?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>S0035-001X2006000900035</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Formación de paredes de dominio en transiciones de fase de primer orden]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[García]]></surname>
<given-names><![CDATA[J. L]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Melfo]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Pantoja]]></surname>
<given-names><![CDATA[N]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad de Los Andes Postgrado en Física Fundamental ]]></institution>
<addr-line><![CDATA[Mérida ]]></addr-line>
<country>Venezuela</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad de Los Andes Centro de Astrofísica Teórica ]]></institution>
<addr-line><![CDATA[Mérida ]]></addr-line>
<country>Venezuela</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<volume>52</volume>
<fpage>123</fpage>
<lpage>126</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2006000900035&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2006000900035&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2006000900035&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se estudia la formación de paredes de dominio en transiciones de fase de primer orden producidas por un campo escalar que rompe espontáneamente una simetría Z2. Se implementa un algoritmo que permite simular la nucleación y colisión de burbujas de la nueva fase, e identificar el número de paredes cerradas y abiertas formadas. Se estudia el caso de simetría Z2 aproximada, relevante en recientes propuestas de solución al problema de las paredes de dominio en un contexto cosmológico.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[We study formation of domain wall in first order phase transition triggered by a scalar field that breaks spontaneously a Z2 symemetry. An algorithm that allows simulation of bubble nucleation and collision, and counting of open and closed walls formed, is implemented. The case of an approximate Z2 symetry, relevant to recent proposals of solutions to the domain wall problem in cosmology is considered.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[Relatividad general]]></kwd>
<kwd lng="es"><![CDATA[defectos topológicos]]></kwd>
<kwd lng="es"><![CDATA[paredes de dominio]]></kwd>
<kwd lng="en"><![CDATA[General relativity]]></kwd>
<kwd lng="en"><![CDATA[topological defects]]></kwd>
<kwd lng="en"><![CDATA[domain walls]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">F&iacute;sica Te&oacute;rica</font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Formaci&oacute;n de paredes de dominio en transiciones de fase de primer orden</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>J. L. Garc&iacute;a*, A. Melfo** y N. Pantoja**</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>* Postgrado en F&iacute;sica Fundamental, Universidad de Los Andes, M&eacute;rida, Venezuela </i></font></p>     <p align="justify"><font face="verdana" size="2"><i>** Centro de Astrof&iacute;sica Te&oacute;rica, Universidad de Los Andes, M&eacute;rida, Venezuela</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 24 de noviembre de 2003    ]]></body>
<body><![CDATA[<br> Aceptado el 5 de junio de 2004</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">Se estudia la formaci&oacute;n de paredes de dominio en transiciones de fase de primer orden producidas por un campo escalar que rompe espont&aacute;neamente una simetr&iacute;a <i>Z<sub>2</sub>. </i>Se implementa un algoritmo que permite simular la nucleaci&oacute;n y colisi&oacute;n de burbujas de la nueva fase, e identificar el n&uacute;mero de paredes cerradas y abiertas formadas. Se estudia el caso de simetr&iacute;a <i>Z<sub>2</sub> </i>aproximada, relevante en recientes propuestas de soluci&oacute;n al problema de las paredes de dominio en un contexto cosmol&oacute;gico.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> Relatividad general; defectos topol&oacute;gicos; paredes de dominio.</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 study formation of domain wall in first order phase transition triggered by a scalar field that breaks spontaneously a <i>Z<sub>2</sub> </i>symemetry. An algorithm that allows simulation of bubble nucleation and collision, and counting of open and closed walls formed, is implemented. The case of an approximate <i>Z<sub>2</sub> </i>symetry, relevant to recent proposals of solutions to the domain wall problem in cosmology is considered.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords:</b> General relativity; topological defects; domain walls.</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:   11.27.+d</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/v52s3/v52s3a35.pdf">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. S. Weinberg, <i>Phys. Rev. D </i><b>9</b> (1974) 3357;    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8326811&pid=S0035-001X200600090003500001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --> L. Dolan y R. Jackiw, <i>Phys. Rev. D </i><b>9 </b>(1974) 3320.</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=8326812&pid=S0035-001X200600090003500002&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. D. Kirzhnits y A. Linde, <i>Phys. Lett. B </i><b>42 </b>(1972) 47.</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=8326813&pid=S0035-001X200600090003500003&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">3. T.W. Kibble, <i>Journal. Phys. A </i><b>9</b> (1976) 1387.</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=8326814&pid=S0035-001X200600090003500004&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">4. T. Vachaspati y A. Vilenkin, <i>Phys. Rev. D </i><b>30</b> (1984).</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=8326815&pid=S0035-001X200600090003500005&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">5. S. Coleman, <i>Phys. Rev. D </i><b>15</b> (1977) 2929.</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=8326816&pid=S0035-001X200600090003500006&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">6. T.W. Kibble, T. Vachaspati y A. Vilenkin, <i>Phys. Rev D </i><b>51</b> (1995) 1934;    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8326817&pid=S0035-001X200600090003500007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --> A. Melfo y L. Perivolaropoulus, <i>Phys. Rev. D </i><b>52 </b>(1995) 992;    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8326818&pid=S0035-001X200600090003500008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><!-- ref --> T. Vachaspati, A. Vilenkin, KIbble y Borrill, <i>Phy.</i><i> Rev.</i></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=8326819&pid=S0035-001X200600090003500009&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">7. Y.B. Zeldovich, I.Y. Kobsareb y L.B. Okun, <i>Soviet Phys. JETP. </i> <b>40</b> (1975).</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=8326820&pid=S0035-001X200600090003500010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
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