<?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>S0035-001X2010000300002</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[New coordinates for the four-body problem]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Piña]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Autónoma Metropolitana Unidad Iztapalapa ]]></institution>
<addr-line><![CDATA[México D.F.]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2010</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2010</year>
</pub-date>
<volume>56</volume>
<numero>3</numero>
<fpage>195</fpage>
<lpage>203</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2010000300002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2010000300002&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2010000300002&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[A new coordinate system is defined to study the physical Four-Body dynamical problem with general masses, with the origin the of coordinates at the center of mass. The transformation from the frame of inertial coordinates involves a combination of a rotation to the system of principal axis of inertia, followed by three changes of scale modifying the principal moments of inertia yield to a body with three equal moments of inertia, and finally a second rotation that leaves unaltered the equal moments of inertia. These three transformation steps yield a mass-dependent, rigid, orthocentric tetrahedron of constant volume in the baricentric inertial coordinates. Each of those three linear transformations is a function of three coordinates that produce the nine degrees of freedom of the Physical Four-Body problem, in a coordinate system with the center of mass as origin. The relation between the well-known equilateral tetrahedron solution to the gravitational Four-Body problem and the new coordinates is exhibited, and the planar case of central configurations with four different masses is computed numerically in these coordinates.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Se define un sistema de coordenadas nuevo para el problema dinámico de cuatro cuerpos con masas diferentes, con origen de coordenadas en el centro de masa. La transformación desde el sistema de coordenadas inercial incluye una combinación de una rotación al sistema de ejes principales de inercia, seguida por tres cambios de escala que modifican los tres momentos principales de inercia para producir un cuerpo con los tres momentos principales de inercia iguales, y finalmente otra rotación que deja inalterados los momentos de inercia iguales. Estas tres transformaciones llevan un tetraedro rígido, ortocéntrico, función de las masas, con tres momentos principales de inercia iguales, de volumen constante al tetraedro que forman las coordenadas inerciales. Cada una de estas tres transformaciones lineales es una función de tres coordenadas que producen los nueve grados de libertad del Problema de Cuatro Cuerpos en este sistema de coordenadas, con el centro de masa en el origen. Se exhibe la relación entre la solución muy conocida de tetrahedro equilátero del problema gravitacional de Cuatro Cuerpos y las coordenadas nuevas, y después el caso plano de configuraciones centrales, con cuatro masas diferentes, se calculó numéricamente en estas coordenadas.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Four-body problem]]></kwd>
<kwd lng="en"><![CDATA[new coordinates]]></kwd>
<kwd lng="es"><![CDATA[Problema de cuatro cuerpos]]></kwd>
<kwd lng="es"><![CDATA[coordenadas nuevas]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Investigaci&oacute;n</font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>New coordinates for the four&#150;body problem</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>E. Pi&ntilde;a</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>Department of Physics, Universidad Aut&oacute;noma Metropolitana &#150; Iztapalapa, P.O. Box 55 534, M&eacute;xico, D.F., 09340 M&eacute;xico, e&#150;mail: </i><a href="mailto:pge@xanum.uam.mx">pge@xanum.uam.mx</a></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 17 de agosto de 2009    <br>   Aceptado el 20 de abril de 2010</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>Abstract</b></font></p>     <p align="justify"><font face="verdana" size="2">A new coordinate system is defined to study the physical Four&#150;Body dynamical problem with general masses, with the origin the of coordinates at the center of mass. The transformation from the frame of inertial coordinates involves a combination of a rotation to the system of principal axis of inertia, followed by three changes of scale modifying the principal moments of inertia yield to a body with three equal moments of inertia, and finally a second rotation that leaves unaltered the equal moments of inertia. These three transformation steps yield a mass&#150;dependent, rigid, orthocentric tetrahedron of constant volume in the baricentric inertial coordinates. Each of those three linear transformations is a function of three coordinates that produce the nine degrees of freedom of the Physical Four&#150;Body problem, in a coordinate system with the center of mass as origin. The relation between the well&#150;known equilateral tetrahedron solution to the gravitational Four&#150;Body problem and the new coordinates is exhibited, and the planar case of central configurations with four different masses is computed numerically in these coordinates.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords:</b>  Four&#150;body problem; new coordinates.</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 define un sistema de coordenadas nuevo para el problema din&aacute;mico de cuatro cuerpos con masas diferentes, con origen de coordenadas en el centro de masa. La transformaci&oacute;n desde el sistema de coordenadas inercial incluye una combinaci&oacute;n de una rotaci&oacute;n al sistema de ejes principales de inercia, seguida por tres cambios de escala que modifican los tres momentos principales de inercia para producir un cuerpo con los tres momentos principales de inercia iguales, y finalmente otra rotaci&oacute;n que deja inalterados los momentos de inercia iguales. Estas tres transformaciones llevan un tetraedro r&iacute;gido, ortoc&eacute;ntrico, funci&oacute;n de las masas, con tres momentos principales de inercia iguales, de volumen constante al tetraedro que forman las coordenadas inerciales. Cada una de estas tres transformaciones lineales es una funci&oacute;n de tres coordenadas que producen los nueve grados de libertad del Problema de Cuatro Cuerpos en este sistema de coordenadas, con el centro de masa en el origen. Se exhibe la relaci&oacute;n entre la soluci&oacute;n muy conocida de tetrahedro equil&aacute;tero del problema gravitacional de Cuatro Cuerpos y las coordenadas nuevas, y despu&eacute;s el caso plano de configuraciones centrales, con cuatro masas diferentes, se calcul&oacute; num&eacute;ricamente en estas coordenadas.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> Problema de cuatro cuerpos; coordenadas nuevas.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">PACS: 45.50.Pk; 95.10.Ce</font></p>     ]]></body>
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