<?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>0120-419X</journal-id>
<journal-title><![CDATA[Revista Integración]]></journal-title>
<abbrev-journal-title><![CDATA[Integración - UIS]]></abbrev-journal-title>
<issn>0120-419X</issn>
<publisher>
<publisher-name><![CDATA[Universidad Industrial de Santander]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0120-419X2011000100005</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Timelike and null equatorial geodesics in the Bonnor-Sackfield relativistic disk]]></article-title>
<article-title xml:lang="es"><![CDATA[Geodésicas tipo tiempo y nulas en el plano ecuatorial del disco relativista de Bonnor-Sackfield]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[GONZÁLEZ]]></surname>
<given-names><![CDATA[GUILLERMO A.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[LÓPEZ-SUSPES]]></surname>
<given-names><![CDATA[FRAMSOL]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Industrial de Santander Escuela de Física ]]></institution>
<addr-line><![CDATA[Bucaramanga ]]></addr-line>
<country>Colombia</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidad Santo Tomás Facultad de Telecomunicaciones ]]></institution>
<addr-line><![CDATA[Bucaramanga ]]></addr-line>
<country>Colombia</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>06</month>
<year>2011</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>06</month>
<year>2011</year>
</pub-date>
<volume>29</volume>
<numero>1</numero>
<fpage>59</fpage>
<lpage>72</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_arttext&amp;pid=S0120-419X2011000100005&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_abstract&amp;pid=S0120-419X2011000100005&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.co/scielo.php?script=sci_pdf&amp;pid=S0120-419X2011000100005&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract. A study of timelike and null equatorial geodesics in the Bonnor- Sackfield relativistic thin disk is presented. The motion of test particles in the equatorial plane is analyzed, both for the newtonian thin disk model as for the corresponding relativistic disk. The nature of the possible orbits is studied by means of a qualitative analysis of the effective potential and by numerically solving the motion equation for radial and non-radial equatorial trajectories. The existence of stable, unstable and marginally stable circular orbits is analyzed, both for the newtonian and relativistic case. Examples of the numerical results, obtained with some simple values of the parameters, are presented.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Resumen. En este trabajo se presenta un estudio de las geodésicas temporales y nulas en el disco delgado relativista y newtoniano de Bonnor-Sackfield. Se analiza el movimiento de las partículas de prueba en el plano ecuatorial, tanto para el modelo newtoniano del disco delgado como para el disco relativista correspondiente. La naturaleza de las órbitas posibles se estudia por medio de un análisis cualitativo del potencial efectivo, y numéricamente mediante la solución de la ecuación de movimiento de las trayectorias ecuatorial radial y no radial: Se analiza la existencia de órbitas estables, circulares inestables y estables marginalmente, tanto para el caso newtoniano, como el relativista. Se presentan ejemplos de los resultados numéricos obtenidos con algunos valores de los parámetros simples.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[General relativity]]></kwd>
<kwd lng="en"><![CDATA[exact solutions]]></kwd>
<kwd lng="en"><![CDATA[equations of motion]]></kwd>
<kwd lng="es"><![CDATA[Relatividad general]]></kwd>
<kwd lng="es"><![CDATA[soluciones exactas]]></kwd>
<kwd lng="es"><![CDATA[ecuaciones de movimiento]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[   <font size="2" face="Verdana">     <p align="center"><font size="4"><i><b>Timelike and null equatorial geodesics in the    <br> Bonnor-Sackfield relativistic disk</b></i></font></p>      <p align="center">GUILLERMO A. GONZ&Aacute;LEZ<sup> a,*</sup>, FRAMSOL L&Oacute;PEZ-SUSPES<sup>a,b</sup></p>      <p align="center"><sup>a</sup> Universidad Industrial de Santander, Escuela de F&iacute;sica, Bucaramanga, Colombia.    <br> <sup>b</sup> Universidad Santo Tom&aacute;s, Facultad de Telecomunicaciones, Bucaramanga, Colombia.    <br> <hr>     <p align="justify"><b><i>Abstract.</i></b> A study of timelike and null equatorial geodesics in the Bonnor- Sackfield relativistic thin disk is presented. The motion of test particles in the equatorial plane is analyzed, both for the newtonian thin disk model as for the corresponding relativistic disk. The nature of the possible orbits is studied by means of a qualitative analysis of the effective potential and by numerically solving the motion equation for radial and non-radial equatorial trajectories. The existence of stable, unstable and marginally stable circular orbits is analyzed, both for the newtonian and relativistic case. Examples of the numerical results, obtained with some simple values of the parameters, are presented.    <br> <b><i>Keywords:</i></b> General relativity, exact solutions, equations of motion.    <br> <b><i>MSC2000:</i></b> 83Cxx, 83C10, 83C15.</p> <hr>     ]]></body>
<body><![CDATA[<p align="center"><font size="3"><b><i>Geod&eacute;sicas tipo tiempo y nulas en el plano ecuatorial    <br> del disco relativista de Bonnor-Sackfield</i></b></font></p>      <p align="justify"><b><i>Resumen.</i></b> En este trabajo se presenta un estudio de las geod&eacute;sicas temporales y nulas en el disco delgado relativista y newtoniano de Bonnor-Sackfield. Se analiza el movimiento de las part&iacute;culas de prueba en el plano ecuatorial, tanto para el modelo newtoniano del disco delgado como para el disco relativista correspondiente. La naturaleza de las &oacute;rbitas posibles se estudia por medio de un an&aacute;lisis cualitativo del potencial efectivo, y num&eacute;ricamente mediante la soluci&oacute;n de la ecuaci&oacute;n de movimiento de las trayectorias ecuatorial radial y no radial: Se analiza la existencia de &oacute;rbitas estables, circulares inestables y estables marginalmente, tanto para el caso newtoniano, como el relativista. Se presentan ejemplos de los resultados num&eacute;ricos obtenidos con algunos valores de los par&aacute;metros simples.    <br> <b><i>Palabras claves:</i></b> Relatividad general, soluciones exactas, ecuaciones de movimiento.</p> <hr>     <p align="justify">Texto Completo disponible en <a href ="pdf\rein\v29n1\v29n1a05.pdf">PDF</a></p> <hr>     <p align="left"><font size="3"><b><i>References</i></b></font>   </p>      <!-- ref --><p align="justify">&#91;1&#93; Bateman H., <i>Higher Transcendental Functions,</i> McGraw Hill, New York, vol 1. 1953.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000019&pid=S0120-419X201100010000500001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;2&#93; Bic&aacute;k J. and Ledvinka T., &quot;Relativistic disks as sources of the Kerr metric&quot;, <i>Phys. Rev. Lett.</i> 71 (1993), no. 11, 1669–1672.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000021&pid=S0120-419X201100010000500002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      ]]></body>
<body><![CDATA[<!-- ref --><p align="justify">&#91;3&#93; Bic&aacute;k J., Lynden-Bell D. and Katz J., &quot;Relativistic disks as sources of static vacuum spacetimes&quot;, <i>Phys. Rev.</i> D 47 (1993), 4334–4343.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000023&pid=S0120-419X201100010000500003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;4&#93; Bic&aacute;k J., Lynden-Bell D. and Pichon C., &quot;Relativistic discs and flat galaxy models&quot;, <i>Monthly Notice Roy Astronom. Soc.</i> 265 (1993), no. 1, 126–144.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000025&pid=S0120-419X201100010000500004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;5&#93; Bonnor W.A. and Sackfield A., &quot;The interpretation of some spheroidal metrics&quot;, <i>Comm. Math. Phys.</i> 8 (1968), no. 4, 338–344.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000027&pid=S0120-419X201100010000500005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;6&#93; D'Afonseca L.A., Letelier P.S., and Oliveira S.R., &quot;Geodesics around Weyl-Bach's ring solution&quot;, <i>Class. Quantum Grav.</i> 22 (2005), no. 17, 3803–3814.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000029&pid=S0120-419X201100010000500006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;7&#93; Gonz&aacute;lez G. and Espitia O.A., &quot;Relativistic static thin disks: The counterrotating model&quot;, <i>Phys. Rev. D</i> 68 (2003), no. 10, 104028-1 – 104028-8.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000031&pid=S0120-419X201100010000500007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      ]]></body>
<body><![CDATA[<!-- ref --><p align="justify">&#91;8&#93; Gonz&aacute;lez G. and Letelier P.S., &quot;Rotating relativistic thin disks&quot;, <i>Phys. Rev. D</i> 62 (2000), 064025-1 – 064025-8.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000033&pid=S0120-419X201100010000500008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;9&#93; Gonz&aacute;lez G. and Letelier P.S., &quot;Relativistic static thin discs with radial stress support&quot;, <i>Class. Quantum Grav.</i> 16 (1999), no. 2, 479–494.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000035&pid=S0120-419X201100010000500009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>     <!-- ref --><p align="justify">&#91;10&#93; Kramer D., Stephani H., Herlt E. and McCallum M., <i>Exact Solutions of Einsteins's Field Equations,</i> Cambridge University Press, Cambridge-England, 2000.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000037&pid=S0120-419X201100010000500010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;11&#93; Lemos J.P.S., &quot;Self-similar relativistic discs with pressure&quot;, <i>Class. Quantum Grav.</i> 6 (1989), no. 9, 1219–1230.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000039&pid=S0120-419X201100010000500011&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;12&#93; Lemos J.P.S. and Letelier P.S., &quot;Superposition of Morgan and Morgan discs with a Schwarzschild black hole&quot;, <i>Class. Quantum Grav.</i> 10 (1993), no. 6, L75–L78.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000041&pid=S0120-419X201100010000500012&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      ]]></body>
<body><![CDATA[<!-- ref --><p align="justify">&#91;13&#93; Lemos J.P.S. and Letelier P.S., &quot;Exact general relativistic thin disks around black holes&quot;, <i>Phys. Rev. D</i> 49 (1994), 5135–5143.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000043&pid=S0120-419X201100010000500013&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;14&#93; Lemos J.P.S. and Letelier P.S., &quot;Two families of exact disks with a central black hole&quot;, <i>Int. J. Modern Phys. D</i> 5 (1996), no. 1, 53–63.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000045&pid=S0120-419X201100010000500014&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;15&#93; Letelier P.S. and Oliveira S.R., &quot;Exact selfgravitating disks and rings: a solitonic approach&quot;, <i>J. Math. Phys.</i> 28 (1987), no. 1, 165–170.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000047&pid=S0120-419X201100010000500015&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;16&#93; Lynden-Bell D. and Pineault S., &quot;Relativistic disks - 1. Counter rotating disks&quot;, <i>Monthly Notice Roy Astronom. Soc.</i> 185 (1978), 679–694.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000049&pid=S0120-419X201100010000500016&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;17&#93; Lynden-Bell D. and Pineault S., &quot;Relativistic disks - 11. Self-similar disks in rotation&quot;, <i>Monthly Notice Roy Astronom. Soc.</i> 185 (1978), 695–712.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000051&pid=S0120-419X201100010000500017&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      ]]></body>
<body><![CDATA[<!-- ref --><p align="justify">&#91;18&#93; Morgan T. and Morgan L., &quot;The Gravitational Field of a Disk&quot;, <i>Phys. Rev.</i> 183 (1969), 1097–1101.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000053&pid=S0120-419X201100010000500018&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;19&#93; Morgan L. and Morgan T., &quot;Gravitational Field of Shells and Disks in General Relativity&quot;, <i>Phys. Rev. D</i> 2 (1970), 2756–2761.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000055&pid=S0120-419X201100010000500019&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;20&#93; Morse P.M. and Feshbach H., <i>Methods of Theoretical Physics,</i> McGraw-Hill, New York, 1953.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000057&pid=S0120-419X201100010000500020&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;21&#93; Semer&aacute;k O., &quot;Gravitating discs around a Schwarzschild black hole. III&quot;, <i>Class. Quantum Grav.</i> 20 (2003), no. 9, 1613–1634.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000059&pid=S0120-419X201100010000500021&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;22&#93; Semer&aacute;k O. and Z&aacute;cek M., &quot;Oscillations of static discs around Schwarzschild black holes: Effect of self-gravitation&quot;, <i>Publ. Astron. Soc. Japan</i> 52 (2000), 1067–1074.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000061&pid=S0120-419X201100010000500022&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      ]]></body>
<body><![CDATA[<!-- ref --><p align="justify">&#91;23&#93; Semer&aacute;k O., Z&aacute;cek M. and Zellerin T., &quot;The structure of superposed Weyl fields&quot;, <i>Monthly Notice Roy Astronom. Soc.</i> 308 (1999), 691–704.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000063&pid=S0120-419X201100010000500023&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>     <!-- ref --><p align="justify">&#91;24&#93; Voorhees B.H., &quot;Static Axially Symmetric Gravitational Fields&quot;, <i>Phys. Rev. D</i> 2 (1970), 2119–2122.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000065&pid=S0120-419X201100010000500024&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;25&#93; Weyl H., &quot;Ausbreitung elektromagnetischer Wellen &uuml;ber einem ebenen Leiter&quot;, <i>Ann. Physik</i> 54 (1917), 117–145.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000067&pid=S0120-419X201100010000500025&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;26&#93; Weyl H., &quot;Bemerkung &uuml;ber die axialsymmetrischen L&ouml;sungen der Einsteinschen Gravitationsgleichungen&quot;, <i>Ann. Physik</i> 59 (1919), 185–189.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000069&pid=S0120-419X201100010000500026&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>      <!-- ref --><p align="justify">&#91;27&#93; Zipoy D.M., &quot;Topology of Some Spheroidal Metrics&quot;, <i>J. Math. Phys.</i> 7 (1966), 1137–1143.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=000071&pid=S0120-419X201100010000500027&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></p>  <hr>     ]]></body>
<body><![CDATA[<p align="justify"><sup>*</sup>Corresponding author: <i>E-mail:</i> <a href="mailto:guillego@uis.edu.co">guillego@uis.edu.co</a>.    <br> <b>Received:</b> 11 March 2010, <b>Accepted:</b> 3 June 2011. </font>      ]]></body><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bateman]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
</person-group>
<source><![CDATA[Higher Transcendental Functions]]></source>
<year>1953</year>
<volume>1</volume>
<publisher-loc><![CDATA[New York ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bicák]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Ledvinka]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic disks as sources of the Kerr metric]]></article-title>
<source><![CDATA[Phys. Rev. Lett.]]></source>
<year>1993</year>
<volume>71</volume>
<numero>11</numero>
<issue>11</issue>
<page-range>1669-1672</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[Bicák]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Lynden-Bell]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Katz]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic disks as sources of static vacuum spacetimes]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>1993</year>
<volume>47</volume>
<page-range>4334-4343</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[Bicák]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Lynden-Bell]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Pichon]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic discs and flat galaxy models]]></article-title>
<source><![CDATA[Monthly Notice Roy Astronom. Soc.]]></source>
<year>1993</year>
<volume>265</volume>
<numero>1</numero>
<issue>1</issue>
<page-range>126-144</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Bonnor]]></surname>
<given-names><![CDATA[W.A.]]></given-names>
</name>
<name>
<surname><![CDATA[Sackfield]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The interpretation of some spheroidal metrics]]></article-title>
<source><![CDATA[Comm. Math. Phys.]]></source>
<year>1968</year>
<volume>8</volume>
<numero>4</numero>
<issue>4</issue>
<page-range>338-344</page-range></nlm-citation>
</ref>
<ref id="B6">
<label>6</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[D'Afonseca]]></surname>
<given-names><![CDATA[L.A.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Oliveira]]></surname>
<given-names><![CDATA[S.R.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Geodesics around Weyl-Bach's ring solution]]></article-title>
<source><![CDATA[Class. Quantum Grav.]]></source>
<year>2005</year>
<volume>22</volume>
<numero>17</numero>
<issue>17</issue>
<page-range>3803-3814</page-range></nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[González]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<name>
<surname><![CDATA[Espitia]]></surname>
<given-names><![CDATA[O.A.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic static thin disks: The counterrotating model]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2003</year>
<volume>68</volume>
<numero>10</numero>
<issue>10</issue>
<page-range>104028-1 - 104028-8</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[González]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Rotating relativistic thin disks]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2000</year>
<volume>62</volume>
<page-range>064025-1 - 064025-8</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[González]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic static thin discs with radial stress support]]></article-title>
<source><![CDATA[Class. Quantum Grav.]]></source>
<year>1999</year>
<volume>16</volume>
<numero>2</numero>
<issue>2</issue>
<page-range>479-494</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[Kramer]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Stephani]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Herlt]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[McCallum]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<source><![CDATA[Exact Solutions of Einsteins's Field Equations]]></source>
<year>2000</year>
<publisher-loc><![CDATA[Cambridge ]]></publisher-loc>
<publisher-name><![CDATA[Cambridge University Press]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B11">
<label>11</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lemos]]></surname>
<given-names><![CDATA[J.P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Self-similar relativistic discs with pressure]]></article-title>
<source><![CDATA[Class. Quantum Grav.]]></source>
<year>1989</year>
<volume>6</volume>
<numero>9</numero>
<issue>9</issue>
<page-range>1219-1230</page-range></nlm-citation>
</ref>
<ref id="B12">
<label>12</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lemos]]></surname>
<given-names><![CDATA[J.P.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Superposition of Morgan and Morgan discs with a Schwarzschild black hole]]></article-title>
<source><![CDATA[Class. Quantum Grav.]]></source>
<year>1993</year>
<numero>10</numero><numero>6</numero>
<issue>10</issue><issue>6</issue>
<page-range>L75-L78</page-range></nlm-citation>
</ref>
<ref id="B13">
<label>13</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lemos]]></surname>
<given-names><![CDATA[J.P.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Exact general relativistic thin disks around black holes]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>1994</year>
<volume>49</volume>
<page-range>5135-5143</page-range></nlm-citation>
</ref>
<ref id="B14">
<label>14</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lemos]]></surname>
<given-names><![CDATA[J.P.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Two families of exact disks with a central black hole]]></article-title>
<source><![CDATA[Int. J. Modern Phys. D]]></source>
<year>1996</year>
<volume>5</volume>
<numero>1</numero>
<issue>1</issue>
<page-range>53-63</page-range></nlm-citation>
</ref>
<ref id="B15">
<label>15</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Letelier]]></surname>
<given-names><![CDATA[P.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Oliveira]]></surname>
<given-names><![CDATA[S.R.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Exact selfgravitating disks and rings: a solitonic approach]]></article-title>
<source><![CDATA[J. Math. Phys.]]></source>
<year>1987</year>
<volume>28</volume>
<numero>1</numero>
<issue>1</issue>
<page-range>165-170</page-range></nlm-citation>
</ref>
<ref id="B16">
<label>16</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lynden-Bell]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Pineault]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic disks - 1.: Counter rotating disks]]></article-title>
<source><![CDATA[Monthly Notice Roy Astronom. Soc.]]></source>
<year>1978</year>
<volume>185</volume>
<page-range>679-694</page-range></nlm-citation>
</ref>
<ref id="B17">
<label>17</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lynden-Bell]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Pineault]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Relativistic disks - 11. Self-similar disks in rotation]]></article-title>
<source><![CDATA[Monthly Notice Roy Astronom. Soc.]]></source>
<year>1978</year>
<volume>185</volume>
<page-range>695-712</page-range></nlm-citation>
</ref>
<ref id="B18">
<label>18</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Morgan]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
<name>
<surname><![CDATA[Morgan]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The Gravitational Field of a Disk]]></article-title>
<source><![CDATA[Phys. Rev.]]></source>
<year>1969</year>
<volume>183</volume>
<page-range>1097-1101</page-range></nlm-citation>
</ref>
<ref id="B19">
<label>19</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Morgan]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[Morgan]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Gravitational Field of Shells and Disks in General Relativity]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>1970</year>
<volume>2</volume>
<page-range>2756-2761</page-range></nlm-citation>
</ref>
<ref id="B20">
<label>20</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Morse]]></surname>
<given-names><![CDATA[P.M.]]></given-names>
</name>
<name>
<surname><![CDATA[Feshbach]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
</person-group>
<source><![CDATA[Methods of Theoretical Physics]]></source>
<year>1953</year>
<publisher-loc><![CDATA[New York ]]></publisher-loc>
<publisher-name><![CDATA[McGraw-Hill]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B21">
<label>21</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Semerák]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Gravitating discs around a Schwarzschild black hole. III]]></article-title>
<source><![CDATA[Class. Quantum Grav.]]></source>
<year>2003</year>
<volume>20</volume>
<numero>9</numero>
<issue>9</issue>
<page-range>1613-1634</page-range></nlm-citation>
</ref>
<ref id="B22">
<label>22</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Semerák]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
<name>
<surname><![CDATA[Zácek]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Oscillations of static discs around Schwarzschild black holes: Effect of self-gravitation]]></article-title>
<source><![CDATA[Publ. Astron. Soc.]]></source>
<year>2000</year>
<volume>52</volume>
<page-range>1067-1074</page-range></nlm-citation>
</ref>
<ref id="B23">
<label>23</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Semerák]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
<name>
<surname><![CDATA[Zácek]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Zellerin]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[The structure of superposed Weyl fields]]></article-title>
<source><![CDATA[Monthly Notice Roy Astronom. Soc.]]></source>
<year>1999</year>
<volume>308</volume>
<page-range>691-704</page-range></nlm-citation>
</ref>
<ref id="B24">
<label>24</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Voorhees]]></surname>
<given-names><![CDATA[B.H.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Static Axially Symmetric Gravitational Fields]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>1970</year>
<volume>2</volume>
<page-range>2119-2122</page-range></nlm-citation>
</ref>
<ref id="B25">
<label>25</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Weyl]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Ausbreitung elektromagnetischer Wellen über einem ebenen Leiter]]></article-title>
<source><![CDATA[Ann. Physik]]></source>
<year>1917</year>
<volume>54</volume>
<page-range>117-145</page-range></nlm-citation>
</ref>
<ref id="B26">
<label>26</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Weyl]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Bemerkung über die axialsymmetrischen Lösungen der Einsteinschen Gravitationsgleichungen]]></article-title>
<source><![CDATA[Ann. Physik]]></source>
<year>1919</year>
<volume>59</volume>
<page-range>185-189</page-range></nlm-citation>
</ref>
<ref id="B27">
<label>27</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Zipoy]]></surname>
<given-names><![CDATA[D.M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Topology of Some Spheroidal Metrics]]></article-title>
<source><![CDATA[J. Math. Phys.]]></source>
<year>1966</year>
<volume>7</volume>
<page-range>1137-1143</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
