<?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>S0035-001X2007001000027</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Regularización de códigos en simetría esférica y axial en relatividad numérica]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Ruiz]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Alcubierre]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Núñez]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Nacional Autónoma de México Instituto de Ciencias Nucleares ]]></institution>
<addr-line><![CDATA[México D.F.]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>08</month>
<year>2007</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>08</month>
<year>2007</year>
</pub-date>
<volume>53</volume>
<fpage>144</fpage>
<lpage>147</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2007001000027&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2007001000027&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2007001000027&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Elegir coordenadas adaptadas para evolucionar espacio-tiempos con alguna simetría, usualmente genera divergencias en las ecuaciones de evolución para las variables geométricas. Por esta razón, los códigos de evolución en relatividad numérica rápidamente se hacen inestables. Presentamos un algoritmo genérico para resolver el problema de la regularización que se puede utilizar directamente en las ecuaciones de evolución y que permite escoger de forma general las variables de norma. Este algoritmo es similar al introducido por Rinne y Stewart dentro del formalismo Z4. Sin embargo, nuestro algoritmo es más general y se puede utilizar en una amplia variedad de sistemas de evolución.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[The use of coordinates adapted to evolving space times with some symmetry is often a source problems, the evolution equations for the geometric quantities have divergences. This problem propagates very fast and makes numerical codes crash. We present a generic algorithm for dealing with the regularization problem that can be used directly on the evolution equations, and which allows very general gauge choices. We explicitly show the regularity of the evolution equations, we describe the corresponding numerical code, and we present several examples clearly showing the regularity of our evolutions.]]></p></abstract>
<kwd-group>
<kwd lng="es"><![CDATA[Relatividad numérica]]></kwd>
<kwd lng="es"><![CDATA[espacio-tiempo esféricamente simétrico]]></kwd>
<kwd lng="es"><![CDATA[espacio-tiempo axialmente simétrico]]></kwd>
<kwd lng="es"><![CDATA[condiciones de regularidad]]></kwd>
<kwd lng="en"><![CDATA[Numerical relativity]]></kwd>
<kwd lng="en"><![CDATA[spherically symmetric space-time]]></kwd>
<kwd lng="en"><![CDATA[axi-symmetric space-time]]></kwd>
<kwd lng="en"><![CDATA[regularity conditions]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="center"><font face="verdana" size="4"><b>Regularizaci&oacute;n de c&oacute;digos en simetr&iacute;a esf&eacute;rica y axial en relatividad num&eacute;rica</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>M. Ruiz, M. Alcubierre y D. N&uacute;&ntilde;ez </b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>Instituto de Ciencias Nucleares, Universidad Nacional Aut&oacute;noma de M&eacute;xico, Apartado Postal 70&#150;543, M&eacute;xico D.F. 04510, M&eacute;xico, e&#150;mail: <a href="mailto:ruizm@nucleares.unam.mx" target="_blank">ruizm@nucleares.unam.mx</a>, <a href="mailto:malcubi@nucleares.unam.mx" target="_blank">malcubi@nucleares.unam.mx</a>, <a href="mailto:nunez@nulceares.unam.mx" target="_blank">nunez@nulceares.unam.mx</a></i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 1 de mayo de 2006    <br>   Aceptado el 1 de noviembre de 2006</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>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">Elegir coordenadas adaptadas para evolucionar espacio&#150;tiempos con alguna simetr&iacute;a, usualmente genera divergencias en las ecuaciones de evoluci&oacute;n para las variables geom&eacute;tricas. Por esta raz&oacute;n, los c&oacute;digos de evoluci&oacute;n en relatividad num&eacute;rica r&aacute;pidamente se hacen inestables. Presentamos un algoritmo gen&eacute;rico para resolver el problema de la regularizaci&oacute;n que se puede utilizar directamente en las ecuaciones de evoluci&oacute;n y que permite escoger de forma general las variables de norma. Este algoritmo es similar al introducido por Rinne y Stewart dentro del formalismo <i>Z4. </i>Sin embargo, nuestro algoritmo es m&aacute;s general y se puede utilizar en una amplia variedad de sistemas de evoluci&oacute;n.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores: </b>Relatividad num&eacute;rica; espacio&#150;tiempo esf&eacute;ricamente sim&eacute;trico; espacio&#150;tiempo axialmente sim&eacute;trico; condiciones de regularidad.</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">The use of coordinates adapted to evolving space times with some symmetry is often a source problems, the evolution equations for the geometric quantities have divergences. This problem propagates very fast and makes numerical codes crash. We present a generic algorithm for dealing with the regularization problem that can be used directly on the evolution equations, and which allows very general gauge choices. We explicitly show the regularity of the evolution equations, we describe the corresponding numerical code, and we present several examples clearly showing the regularity of our evolutions.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Numerical relativity; spherically symmetric space&#150;time; axi&#150;symmetric space&#150;time; regularity conditions.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">PACS: 04.20.Ex; 04.25.Dm; 95.30.Sf</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/v53s4/v53s4a27.pdf">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Agradecimientos</b></font></p>     <p align="justify"><font face="verdana" size="2">Este trabajo fue financiado en parte por CONACyT con proyecto SEP&#150;2004&#150;C01&#150;47209, por DGAPA&#150;UNAM con proyecto IN112401 y IN122002, y por DGEP&#150;UNAM con un proyecto complementario.</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. J. Bardeen y T. Piran, <i>Phys. Rep. </i><b>196 </b>(1983) 205.</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=8394937&pid=S0035-001X200700100002700001&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. M.W. Choptuik, <i>Phys. Rev. D </i><b>44</b> (1991) 3124.</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=8394938&pid=S0035-001X200700100002700002&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. M. Alcubierre y J. Gonz&aacute;lez, <i>Comp. Phys. Commun. </i><b>167</b> (2005) 76.</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=8394939&pid=S0035-001X200700100002700003&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. O. Rinne y J.M. Steward, <i>Class. Quantum Grav </i><b>22</b> (2005) 1143.</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=8394940&pid=S0035-001X200700100002700004&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. R. Arnowitt, S. Deser y C.W. Misner, en Gravitation: <i>An Introduction to Current Research, </i>editado por L. Witten (John Wiley, New York, 1962) p. 227.</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=8394941&pid=S0035-001X200700100002700005&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. J. York, en Sources of Gravitational Radiation, editado por L. Smarr (Cam. Univ. Press, Cambridge, England, 1979).</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=8394942&pid=S0035-001X200700100002700006&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. M. Alcubierre <i>et al., Phys. Rev. D </i><b>72</b> (2005) 7124018.</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=8394943&pid=S0035-001X200700100002700007&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">8. C. Bona, J.Mass&oacute;, E. Seidel y J. Stela, PHYS. REV. LETT. <b>75</b> (1995) 600.</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=8394944&pid=S0035-001X200700100002700008&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">9. G. Nagy, O.Ortiz y O. Reula, <i>Phys. Rev. D </i><b>70</b> (2004) 044012.</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=8394945&pid=S0035-001X200700100002700009&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">10. A. Gustafsson, H. Kreiss y J. Oliger, en <i>Time Dependent Problems and Diference Methods, </i>editado por D. Levy (John Wiley, New York, 1995).</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=8394946&pid=S0035-001X200700100002700010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bardeen]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[Piran]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rep]]></source>
<year>1983</year>
<numero>196</numero>
<issue>196</issue>
<page-range>205</page-range></nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[W. Choptuik]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rev]]></source>
<year>1991</year>
<numero>D 44</numero>
<issue>D 44</issue>
<page-range>3124</page-range></nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Alcubierre]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<name>
<surname><![CDATA[González]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<source><![CDATA[Comp. Phys. Commun]]></source>
<year>2005</year>
<numero>167</numero>
<issue>167</issue>
<page-range>76</page-range></nlm-citation>
</ref>
<ref id="B4">
<label>4</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Rinne]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[M. Steward]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<source><![CDATA[Class. Quantum Grav]]></source>
<year>2005</year>
<numero>22</numero>
<issue>22</issue>
<page-range>1143</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Arnowitt]]></surname>
<given-names><![CDATA[R]]></given-names>
</name>
<name>
<surname><![CDATA[Deser]]></surname>
<given-names><![CDATA[S]]></given-names>
</name>
<name>
<surname><![CDATA[W. Misner]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
</person-group>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Witten]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
</person-group>
<source><![CDATA[Gravitation: An Introduction to Current Research]]></source>
<year>1962</year>
<page-range>227</page-range><publisher-loc><![CDATA[New York ]]></publisher-loc>
<publisher-name><![CDATA[John Wiley]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B6">
<label>6</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[York]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Smarr]]></surname>
<given-names><![CDATA[L]]></given-names>
</name>
</person-group>
<source><![CDATA[Sources of Gravitational Radiation]]></source>
<year>1979</year>
<publisher-loc><![CDATA[Cambridge ]]></publisher-loc>
<publisher-name><![CDATA[Cam. Univ. Press]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Alcubierre]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rev]]></source>
<year>2005</year>
<numero>D 72</numero>
<issue>D 72</issue>
<page-range>7124018</page-range></nlm-citation>
</ref>
<ref id="B8">
<label>8</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bona]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<name>
<surname><![CDATA[Massó]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<name>
<surname><![CDATA[Seidel]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<name>
<surname><![CDATA[Stela]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<source><![CDATA[PHYS. REV. LETT]]></source>
<year>1995</year>
<numero>75</numero>
<issue>75</issue>
<page-range>600</page-range></nlm-citation>
</ref>
<ref id="B9">
<label>9</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Nagy]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
<name>
<surname><![CDATA[Ortiz]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
<name>
<surname><![CDATA[Reula]]></surname>
<given-names><![CDATA[O]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rev]]></source>
<year>2004</year>
<numero>D 70</numero>
<issue>D 70</issue>
<page-range>044012</page-range></nlm-citation>
</ref>
<ref id="B10">
<label>10</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Gustafsson]]></surname>
<given-names><![CDATA[A]]></given-names>
</name>
<name>
<surname><![CDATA[Kreiss]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
<name>
<surname><![CDATA[Oliger]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
</person-group>
<person-group person-group-type="editor">
<name>
<surname><![CDATA[Levy]]></surname>
<given-names><![CDATA[D]]></given-names>
</name>
</person-group>
<source><![CDATA[Time Dependent Problems and Diference Methods]]></source>
<year>1995</year>
<publisher-loc><![CDATA[New York ]]></publisher-loc>
<publisher-name><![CDATA[John Wiley]]></publisher-name>
</nlm-citation>
</ref>
</ref-list>
</back>
</article>
