<?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>1870-3542</journal-id>
<journal-title><![CDATA[Revista mexicana de física E]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fís. E]]></abbrev-journal-title>
<issn>1870-3542</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1870-35422008000100005</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Simple deductions of the integral representations of the relativistic Faraday and Ampère-Maxwell laws and the relativistic transformation laws of the electromagnetic field]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Ortiz-Domínguez]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Pereyra]]></surname>
<given-names><![CDATA[E.M]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Ares de Parga]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Instituto Politécnico Nacional Escuela Superior de Física y Matemáticas Depto. de Física]]></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>2008</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2008</year>
</pub-date>
<volume>54</volume>
<numero>1</numero>
<fpage>32</fpage>
<lpage>36</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S1870-35422008000100005&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S1870-35422008000100005&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S1870-35422008000100005&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[By using simple concepts of special relativity and the differential representations of the Faraday and Ampère-Maxwell laws, we deduce their Gelman-Monsivais integral representation. The relativistic transformation laws of the electromagnetic field are also obtained without using tensorial analysis or covariant concepts]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Usando conceptos simples de la relatividad especial y las representaciones diferenciales de las ecuaciones de Faraday y Ampère-Maxwell, se deducen las representaciones integrales de Gelman-Monsivais de estas ultimas. Se obtienen al mismo tiempo las leyes de las transformaciones relativistas del campo electromagnético sin utilizar análisis tensorial o conceptos covariantes]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Special relativity]]></kwd>
<kwd lng="en"><![CDATA[Maxwell equations]]></kwd>
<kwd lng="en"><![CDATA[integral representation]]></kwd>
<kwd lng="es"><![CDATA[Relatividad especial]]></kwd>
<kwd lng="es"><![CDATA[ecuaciones de Maxwell]]></kwd>
<kwd lng="es"><![CDATA[representación integral]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Ense&ntilde;anza</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Simple deductions of the integral representations of the relativistic Faraday and Amp&egrave;re&#150;Maxwell laws and the relativistic transformation laws of the electromagnetic field</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>M. Ortiz&#150;Dom&iacute;nguez, E.M. Pereyra, and G. Ares de Parga</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>Depto. de F&iacute;sica, Escuela Superior de F&iacute;sica y Matem&aacute;ticas, </i><i>Instituto Polit&eacute;cnico Nacional, U.P. Adolfo L&oacute;pez Mateos, Zacatenco, </i><i>07738, M&eacute;xico D.F, M&eacute;xico.</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 14 de mayo de 2007    <br> Aceptado el 4 de septiembre de 2007</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">By using simple concepts of special relativity and the differential representations of the Faraday and Amp&egrave;re&#150;Maxwell laws, we deduce their Gelman&#150;Monsivais integral representation. The relativistic transformation laws of the electromagnetic field are also obtained without using tensorial analysis or covariant concepts.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Special relativity; Maxwell equations; integral representation.</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">Usando conceptos simples de la relatividad especial y las representaciones diferenciales de las ecuaciones de Faraday y Amp&egrave;re&#150;Maxwell, se deducen las representaciones integrales de Gelman&#150;Monsivais de estas ultimas. Se obtienen al mismo tiempo las leyes de las transformaciones relativistas del campo electromagn&eacute;tico sin utilizar an&aacute;lisis tensorial o conceptos covariantes.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores: </b>Relatividad especial; ecuaciones de Maxwell; representaci&oacute;n integral. </font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">PACS: 03.50.De</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmfe/v54n1/v54n1a5.pdf" target="_blank">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>Acknowledgement</b></font></p>     <p align="justify"><font face="verdana" size="2">This work was partially supported by COFAA and EDI &#150; IPN. We thank a referee for valuable and enlightened comments.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. G. Ares de Parga and M.A. Rosales, <i>Eur. J. Phys. </i><b>10</b> (1989) 74.</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=8496422&pid=S1870-3542200800010000500001&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. T. Frankel, <i>Gravitational Curvature. An introduction to Einstein's Theory </i>(San Francisco, Freeman, 1979) Chap. 6 pp. 64.</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=8496423&pid=S1870-3542200800010000500002&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. H. Gelman, <i>Eur. J. Phys. </i><b>12 </b>(1991) 230.</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=8496424&pid=S1870-3542200800010000500003&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. G. Monsivais, <i>Am. J. Phys. </i><b>72 </b>(2004) 1178.</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=8496425&pid=S1870-3542200800010000500004&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. W.K. Panofski and M. Phillips, <i>Classical Electricity and Mag<i>netism, </i></i>2nd edn (Reading, Addison&#150;Wesley, 1962) Chap 9.</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=8496426&pid=S1870-3542200800010000500005&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[Ares de Parga]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
<name>
<surname><![CDATA[Rosales]]></surname>
<given-names><![CDATA[M.A]]></given-names>
</name>
</person-group>
<source><![CDATA[Eur. J. Phys]]></source>
<year>1989</year>
<numero>10</numero>
<issue>10</issue>
<page-range>74</page-range></nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Frankel]]></surname>
<given-names><![CDATA[T]]></given-names>
</name>
</person-group>
<source><![CDATA[Gravitational Curvature: An introduction to Einstein's Theory]]></source>
<year>1979</year>
<page-range>64</page-range><publisher-loc><![CDATA[San Francisco ]]></publisher-loc>
<publisher-name><![CDATA[Freeman]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Gelman]]></surname>
<given-names><![CDATA[H]]></given-names>
</name>
</person-group>
<source><![CDATA[Eur. J. Phys]]></source>
<year>1991</year>
<numero>12</numero>
<issue>12</issue>
<page-range>230</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[Monsivais]]></surname>
<given-names><![CDATA[G]]></given-names>
</name>
</person-group>
<source><![CDATA[Am. J. Phys]]></source>
<year>2004</year>
<numero>72</numero>
<issue>72</issue>
<page-range>1178</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[Panofski]]></surname>
<given-names><![CDATA[W.K]]></given-names>
</name>
<name>
<surname><![CDATA[Phillips]]></surname>
<given-names><![CDATA[M]]></given-names>
</name>
</person-group>
<source><![CDATA[Classical Electricity and Magnetism]]></source>
<year>1962</year>
<edition>2</edition>
<publisher-name><![CDATA[Addison-Wesley]]></publisher-name>
</nlm-citation>
</ref>
</ref-list>
</back>
</article>
