<?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>S0035-001X2021000100007</article-id>
<article-id pub-id-type="doi">10.31349/revmexfis.67.62</article-id>
<title-group>
<article-title xml:lang="es"><![CDATA[Generalización de las transformaciones de Lorentz]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Ortiz Sánchez]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Instituto de Educación Secundaria  ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>España</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>02</month>
<year>2021</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>02</month>
<year>2021</year>
</pub-date>
<volume>67</volume>
<numero>1</numero>
<fpage>62</fpage>
<lpage>67</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2021000100007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2021000100007&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2021000100007&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen En el marco de la relatividad especial, existen numerosos modelos que permiten relacionar el marco de referencia inercial con otro marco de referencia acelerado (no inercial). Vamos a proporcionar las condiciones necesarias y suficientes que determinarán la transformación óptima de una manera única.]]></p></abstract>
<abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract Within the framework of special relativity, there are numerous models that allow an inertial reference frame to be related to another accelerated (non-inertial) reference frame. We are going to provide necessary and sufficient conditions that will determine the optimal transformation in a unique way.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Lorentz]]></kwd>
<kwd lng="en"><![CDATA[non-inertial]]></kwd>
<kwd lng="en"><![CDATA[acceleration]]></kwd>
<kwd lng="es"><![CDATA[Lorentz]]></kwd>
<kwd lng="es"><![CDATA[no inercial]]></kwd>
<kwd lng="es"><![CDATA[aceleración]]></kwd>
</kwd-group>
</article-meta>
</front><back>
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</article>
