<?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>S0035-001X2006000900065</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Landau damping in bi-dust ion-acoustic waves]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Castro]]></surname>
<given-names><![CDATA[E]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Puerta]]></surname>
<given-names><![CDATA[J]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Martín]]></surname>
<given-names><![CDATA[P]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Cereceda]]></surname>
<given-names><![CDATA[C]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Universidad Simón Bolivar Departamento de Fisica ]]></institution>
<addr-line><![CDATA[Caracas ]]></addr-line>
<country>Venezuela</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>05</month>
<year>2006</year>
</pub-date>
<volume>52</volume>
<fpage>224</fpage>
<lpage>226</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2006000900065&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2006000900065&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2006000900065&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Ion acoustic dust waves in a bi-dust plasma are analyzed in this paper. In order to model this system, we assume the existence of two different kinds of grains, each characterized by a different radius. Relative velocities between grains and charge fluctuations are neglected. In order to derive the dispersion relation of this system, we use the well known hybrid fluid-kinetic model, in which ions are treated kinetically and other species as fluids. In this plasma, waves with non-relative velocities between species leads to damped waves with frequency modes, defined by the grain radius. The induced damping ratio is studied as a function of the grain and ion densities.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[En el presente trabajo, analizamos ondas iónico-acústicas de polvo en un plasma con dos tipos de polvo. Para modelar este sistema, asumimos la existencia de dos tipos diferentes de grano, cada uno caracterizado por un diferente radio. Velocidades relativas entre granos y fluctuaciones de cargas son despreciadas. Para derivar la relación de dispersión de este sistema, usamos el bien conocido modelo híbrido fluido-cinético, en el cual los iones son tratados con teoría cinética y las otras especies como fluidos. En este plasma, las ondas sin velocidad relativa entre las especies conducen a ondas amortiguadas con modos de frecuencia definidos por el radio del grano. La razón de amortiguamiento inducido es estudiada en función de las densidades de los granos y de los iones.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Dusty plasmas]]></kwd>
<kwd lng="es"><![CDATA[Plasmas granulares]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="justify"><font face="verdana" size="4">Plasmas</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="4"><b>Landau damping in bi&#150;dust ion&#150;acoustic waves</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>E. Castro, J. Puerta, P. Mart&iacute;n, and C. Cereceda</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i>Universidad Sim&oacute;n Bolivar, Departamento de Fisica, Apartado 89000, Caracas 1080A, Venezuela</i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Recibido el 13 de enero de 2004    <br> Aceptado el 21 de julio de 2004</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">Ion acoustic dust waves in a bi&#150;dust plasma are analyzed in this paper. In order to model this system, we assume the existence of two different kinds of grains, each characterized by a different radius. Relative velocities between grains and charge fluctuations are neglected. In order to derive the dispersion relation of this system, we use the well known hybrid fluid&#150;kinetic model, in which ions are treated kinetically and other species as fluids. In this plasma, waves with non&#150;relative velocities between species leads to damped waves with frequency modes, defined by the grain radius. The induced damping ratio is studied as a function of the grain and ion densities.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Dusty plasmas.</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">En el presente trabajo, analizamos ondas i&oacute;nico&#150;ac&uacute;sticas de polvo en un plasma con dos tipos de polvo. Para modelar este sistema, asumimos la existencia de dos tipos diferentes de grano, cada uno caracterizado por un diferente radio. Velocidades relativas entre granos y fluctuaciones de cargas son despreciadas. Para derivar la relaci&oacute;n de dispersi&oacute;n de este sistema, usamos el bien conocido modelo h&iacute;brido fluido&#150;cin&eacute;tico, en el cual los iones son tratados con teor&iacute;a cin&eacute;tica y las otras especies como fluidos. En este plasma, las ondas sin velocidad relativa entre las especies conducen a ondas amortiguadas con modos de frecuencia definidos por el radio del grano. La raz&oacute;n de amortiguamiento inducido es estudiada en funci&oacute;n de las densidades de los granos y de los iones.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> Plasmas granulares.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">PACS: 52.27. Lw</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/rmf/v52s3/v52s3a65.pdf">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>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. P.K. Shukla, <i>Phys. Plasmas </i><b>8</b> (2001) 1791.</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=8328583&pid=S0035-001X200600090006500001&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. P.K. Shukla and A.A. Mamun, <i>Introduction to Dusty Plasma Physics </i>(IOP Publishing Ltd, London 2002) Chap. 4.</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=8328584&pid=S0035-001X200600090006500002&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. J. Puerta, J. Silva, and C. Cereceda, <i>ICPP 2002. AIP Conf. Prod </i><b>669 </b>(2002) 540.</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=8328585&pid=S0035-001X200600090006500003&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. J. Vranjes, B.P Pandey, and S. Poedts, <i>Phys. Plasmas </i><b>9</b> (2002) 1464.</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=8328586&pid=S0035-001X200600090006500004&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. C. Cereceda, J. Puerta, and P. Mart&iacute;n, <i>Physica Scripta </i><b>T84 </b>(2000) 206.</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=8328587&pid=S0035-001X200600090006500005&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. Puerta, C. Cereceda, Astr. <i>and Space Sci. </i><b>256 </b>(1998) 349.</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=8328588&pid=S0035-001X200600090006500006&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. S.K. El&#150;Labany and W.M. Moslem, <i>Phys. Plasmas </i><b>10</b>  (2003) 4217.</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=8328589&pid=S0035-001X200600090006500007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --> ]]></body><back>
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