<?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>S0035-001X2005000600003</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Two-dimensional treesph simulations of choked flow systems]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Klapp]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sigalotti]]></surname>
<given-names><![CDATA[L. Di G.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Galindo]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Sira]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Instituto Nacional de Investigaciones Nucleares Departamento de Física ]]></institution>
<addr-line><![CDATA[Toluca Estado de México]]></addr-line>
<country>México</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Instituto Venezolano de Investigaciones Científicas Centro de Física ]]></institution>
<addr-line><![CDATA[Caracas Distrito Federal]]></addr-line>
<country>Venezuela</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2005</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2005</year>
</pub-date>
<volume>51</volume>
<numero>6</numero>
<fpage>563</fpage>
<lpage>573</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2005000600003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2005000600003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2005000600003&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[It is well-known that the flow of gas, liquid, and their mixtures through restrictors installed in pipeline systems is of great practical importance in many industrial processes. In spite of its significance, numerical hydrodynamics simulations of such flows are almost non-existent in the literature. Here we present exploratory two-dimensional calculations of the flow of a viscous, single-phase fluid through a wellhead choke of real dimensions, using the method of Smoothed Particle Hydrodynamics (SPH) coupled with a simple isothermal equation of state for description of the flow. The results indicate that an approximately stationary mean flow pattern is rapidly established across the entire tube, with the density and pressure dropping and the flow velocity rising within the choke throat. If the downstream flow is inhibited at the outlet end of the tube, a pressure drop of about 12% occurs across the choke when the mean flow reaches an approximate steady state. If, on the other hand, the flow is not inhibited downstream, the pressure drop is reduced to about 8% or less. The flow across the choke throat remains subsonic with typical velocities of ~ 0.1c, where c denotes the sound speed. In contrast, the flow velocities in the upstream and downstream sections of the pipe are on the average factors of ~ 6 and ~ 3.5 times lower, respectively. Correlation studies based on experimental data indicate that the pressure drop is only 3% or even less for gas flow through wellhead chokes at a speed of 0.1c. This discrepancy reflects the inadequacy of the isothermal equation of state to describe realistic gas flows.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[Es bien conocido que el flujo de gas, líquido y sus mezclas a través de restrictores instalados en sistemas de tuberías es de gran importancia práctica en muchos procesos industriales. A pesar de su importancia, simulaciones hidrodinámicas numéricas de este tipo de flujos son casi inexistentes en la literatura. Aquí presentamos cálculos exploratorios bidimensionales de flujo viscoso de una sola fase a través de un estrangulador de dimensiones reales, utilizando el Método de Hidrodinámica de Partículas Suavizadas (SPH) acoplado con una ecuación sencilla isotérmica de estado para la descripción del flujo. Los resultados indican que un patrón de flujo medio aproximadamente estacionario se establece rápidamente a través de todo el tubo, con la densidad y presión cayendo y el flujo de velocidad aumentando dentro del estrangulador. Si el flujo aguas abajo es inhibido a la salida del tubo, una caída de presión de alrededor de 12% ocurre a través del estrangulador cuando el flujo medio alcanza un estado aproximadamente estacionario. Si, por otro lado, el flujo no es inhibido aguas abajo, la caída de presión se reduce a 8% o menos. El flujo a través del estrangulador se mantiene subsónico con velocidades típicas de ~ 0.1c, donde c denota la velocidad del sonido. En contraste, la velocidad del flujo en las secciones aguas arriba y abajo del tubo son en promedio factores de ~ 6 y ~ 3.5 veces menores, respectivamente. Estudios de correlación basados en datos experimentales indican que la caída de presión es de solo 3% o inclusive menos para flujo de gas a través del estrangulador de la cabeza de un pozo a una velocidad de 0.1c. Esta discrepancia refleja que la ecuación isotérmica de estado no es adecuada para describir flujos realistas de gas.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[SPH]]></kwd>
<kwd lng="en"><![CDATA[numerical particle metnods]]></kwd>
<kwd lng="en"><![CDATA[choked flow]]></kwd>
<kwd lng="en"><![CDATA[compressible flow]]></kwd>
<kwd lng="es"><![CDATA[SPH]]></kwd>
<kwd lng="es"><![CDATA[métodos numéricos de partículas]]></kwd>
<kwd lng="es"><![CDATA[flujo estrangulado]]></kwd>
<kwd lng="es"><![CDATA[flujo compresible]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[  	    <p align="justify"><font face="verdana" size="4">Investigaci&oacute;n</font></p>      <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="4"><b>Two&#45;dimensional treesph simulations of choked flow systems</b></font></p>      <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="center"><font face="verdana" size="2"><b>J. Klapp<sup> a,1</sup>, L. Di G. Sigalotti<sup> b</sup><sup>,</sup><sup>2</sup>, S. Galindo<sup> a</sup><sup>,3</sup>, and E. Sira<sup> b</sup><sup>,</sup><sup>4</sup></b></font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><i><sup>a</sup> Departamento de F&iacute;sica, Instituto Nacional de Investigaciones Nucleares, Km. 36.5 Carretera M&eacute;xico&#45;Toluca, 52045 Estado de M&eacute;xico, M&eacute;xico.</i></font></p>  	    <p align="justify"><font face="verdana" size="2"><i><sup>b</sup> Centro de F&iacute;sica, Instituto Venezolano de Investigaciones Cient&iacute;ficas, Apartado Postal 21827, Caracas 1020A, Venezuela. e&#45;mail: <sup>1 </sup></i><a href="mailto:klapp@nuclear.inin.mx">klapp@nuclear.inin.mx</a><i>,<sup>2 </sup></i><a href="mailto:lsigalot@cassini.ivic.ve">lsigalot@cassini.ivic.ve</a><i>,<sup>3 </sup></i><a href="mailto:sgu@nuclear.inin.mx">sgu@nuclear.inin.mx</a><i>,<sup>4 </sup></i><sup></sup><a href="mailto:esira@hubble.ivic.ve">esira@hubble.ivic.ve</a><i>.</i></font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">Recibido el 1 de septiembre de 2004.    <br>Aceptado el 19 de agosto de 2005.</font></p>      <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">It is well&#45;known that the flow of gas, liquid, and their mixtures through restrictors installed in pipeline systems is of great practical importance in many industrial processes. In spite of its significance, numerical hydrodynamics simulations of such flows are almost non&#45;existent in the literature. Here we present exploratory two&#45;dimensional calculations of the flow of a viscous, single&#45;phase fluid through a wellhead choke of real dimensions, using the method of Smoothed Particle Hydrodynamics (SPH) coupled with a simple isothermal equation of state for description of the flow. The results indicate that an approximately stationary mean flow pattern is rapidly established across the entire tube, with the density and pressure dropping and the flow velocity rising within the choke throat. If the downstream flow is inhibited at the outlet end of the tube, a pressure drop of about 12&#37; occurs across the choke when the mean flow reaches an approximate steady state. If, on the other hand, the flow is not inhibited downstream, the pressure drop is reduced to about 8&#37; or less. The flow across the choke throat remains subsonic with typical velocities of &#126; 0.1<i>c</i>, where <i>c</i> denotes the sound speed. In contrast, the flow velocities in the upstream and downstream sections of the pipe are on the average factors of &#126; 6 and &#126; 3.5 times lower, respectively. Correlation studies based on experimental data indicate that the pressure drop is only 3&#37; or even less for gas flow through wellhead chokes at a speed of 0.1<i>c</i>. This discrepancy reflects the inadequacy of the isothermal equation of state to describe realistic gas flows.</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>Keywords:</b> SPH; numerical particle metnods; choked flow; compressible flow.</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">Es bien conocido que el flujo de gas, l&iacute;quido y sus mezclas a trav&eacute;s de restrictores instalados en sistemas de tuber&iacute;as es de gran importancia pr&aacute;ctica en muchos procesos industriales. A pesar de su importancia, simulaciones hidrodin&aacute;micas num&eacute;ricas de este tipo de flujos son casi inexistentes en la literatura. Aqu&iacute; presentamos c&aacute;lculos exploratorios bidimensionales de flujo viscoso de una sola fase a trav&eacute;s de un estrangulador de dimensiones reales, utilizando el M&eacute;todo de Hidrodin&aacute;mica de Part&iacute;culas Suavizadas (SPH) acoplado con una ecuaci&oacute;n sencilla isot&eacute;rmica de estado para la descripci&oacute;n del flujo. Los resultados indican que un patr&oacute;n de flujo medio aproximadamente estacionario se establece r&aacute;pidamente a trav&eacute;s de todo el tubo, con la densidad y presi&oacute;n cayendo y el flujo de velocidad aumentando dentro del estrangulador. Si el flujo aguas abajo es inhibido a la salida del tubo, una ca&iacute;da de presi&oacute;n de alrededor de 12&#37; ocurre a trav&eacute;s del estrangulador cuando el flujo medio alcanza un estado aproximadamente estacionario. Si, por otro lado, el flujo no es inhibido aguas abajo, la ca&iacute;da de presi&oacute;n se reduce a 8&#37; o menos. El flujo a trav&eacute;s del estrangulador se mantiene subs&oacute;nico con velocidades t&iacute;picas de &#126; 0.1<i>c</i>, donde <i>c</i> denota la velocidad del sonido. En contraste, la velocidad del flujo en las secciones aguas arriba y abajo del tubo son en promedio factores de &#126; 6 y &#126; 3.5 veces menores, respectivamente. Estudios de correlaci&oacute;n basados en datos experimentales indican que la ca&iacute;da de presi&oacute;n es de solo 3&#37; o inclusive menos para flujo de gas a trav&eacute;s del estrangulador de la cabeza de un pozo a una velocidad de 0.1<i>c</i>. Esta discrepancia refleja que la ecuaci&oacute;n isot&eacute;rmica de estado no es adecuada para describir flujos realistas de gas.</font></p>  	    <p align="justify"><font face="verdana" size="2"><b>Descriptores:</b> SPH; m&eacute;todos num&eacute;ricos de part&iacute;culas; flujo estrangulado; flujo compresible.</font></p>  	    ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2">PACS: 47.11.&#43;j;47.27.&#45;i;47.85.Dh</font></p>  	    <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>  	    <p align="justify"><font face="verdana" size="2"><a href="/pdf/rmf/v51n6/v51n6a3.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>Acknowledgments</b></font></p>  	    <p align="justify"><font face="verdana" size="2">We thank an anonymous referee for suggestions that improved the final version of the manuscript. One of us (J.K.) is grateful to Federico Gonzalez Tamez of PEMEX, who introduced me to the interesting problem of flow through wellhead chokes. The calculations in this paper were performed using the Silicon Graphics Altix 350 computer system of the Instituto Nacional de Investigaciones Nucleares (ININ) of Mexico. This work is partially supported by the Mexican Consejo Nacional de Ciencia y Tecnolog&iacute;a (CONACyT) under contracts U43534&#45;R and J200.476/2004, the Fondo Nacional de Ciencia, Tecnolog&iacute;a e Innovation (Fonacit) of Venezuela, the German Deutsche Forshungsgemainshaft (DFG) and the German Deutscher Akademischer Austauschdienst (DAAD).</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. N.C.J. Ros, <i>Appl. Sci. Rev.</i> <b>9</b> (1960) 374.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315257&pid=S0035-001X200500060000300001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">2. F. Fortunati, "Two&#45;phase flow through wellhead chokes", in The SPE&#45;European Spring Meeting 1972 of the Society of Petroleum Engineers of AIME, SPE 3742, (Amsterdam, The Netherlands, May 1972) p. 16.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315259&pid=S0035-001X200500060000300002&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">3. F.E. Ashford, <i>J. Pet. Tech.</i> (1974) August 843.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315261&pid=S0035-001X200500060000300003&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">4. F.E. Ashford and P.E. Pierce, <i>J. Pet. Tech.</i> September (1975) 1145.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315263&pid=S0035-001X200500060000300004&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">5. G.H. Abdul&#45;Majeed, "Correlations developed to predict two phase flow through wellhead chokes", in The 1988 Petroleum Society of CIM, Annual Technical Meeting, CIM 88&#45;39&#45;26, Calgary, (Canada, June 1988) p. 12.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315265&pid=S0035-001X200500060000300005&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">6. T.K. Perkins, <i>SPE Drilling &#38; Completion</i> December (1993) 271.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315267&pid=S0035-001X200500060000300006&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">7. J. Klapp, G. Mendoza, L. Di G. Sigalotti, and E. Sira, "Numerical simulations of flow through wellhead chokes with the Smoothed Particle Hydrodynamics method", in 7th World Conference on Systematics, Cybernetics and Informatics, SCI 2003, (Orlando, USA, July 2003) p. 27.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315269&pid=S0035-001X200500060000300007&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">8. L. Hernquist and N. Katz, <i>Astrophys. J.</i> <b>70</b> (1989) 419.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315271&pid=S0035-001X200500060000300008&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">9. L. Di G. Sigalotti, J. Klapp, E. Sira, Y. Melean, and A. Hasmy, <i>J. Comp. Phys.</i> <b>191</b> (2003) 622.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315273&pid=S0035-001X200500060000300009&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">10. L.D. Libersky, A.G. Petschek, T.C. Carney, J.R. Hipp, and F.A. Allahdadi, <i>J. Comp. Phys.</i> <b>109</b> (1993) 67.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315275&pid=S0035-001X200500060000300010&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">11. O. Flebbe, S. M&uuml;nzel, H. Herold, H. Riffert, and H. Ruder, <i>Astrophys. J.</i> <b>431</b> (1994) 754.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315277&pid=S0035-001X200500060000300011&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">12. S.J. Watkins, A.S. Bhattal, N. Francis, J.A. Turner, and A.P. Whitworth, <i>Astron. Astrophys. Suppl. Ser.</i> <b>119</b> (1996) 177.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315279&pid=S0035-001X200500060000300012&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">13. J.P. Morris, P.J. Fox, and Y. Zhu, <i>J. Comp. Phys.</i> <b>136</b> (1997) 214.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315281&pid=S0035-001X200500060000300013&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">14. J. Bonet and T.&#45;S.L. Lok, <i>Comp. Meth. Appl. Mech. Eng.</i> <b>180</b> (1999) 97.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315283&pid=S0035-001X200500060000300014&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">15. L.D. Sigalotti, H. L&oacute;pez, A. Donoso, E. Sira, and J. Klapp, <i>J. Comp. Phys.</i> <b>212</b> (2006) 124.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315285&pid=S0035-001X200500060000300015&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">16. L.D. Sigalotti and J. Klapp, <i>International Journal of Modern Physics D</i><b> 10</b> (2001) 115.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315287&pid=S0035-001X200500060000300016&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">17. H. Takeda, S.M. Miyama, and M. Sekiya, <i>Prog. Theoret. Phys.</i> <b>92</b> (1994) 939.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315289&pid=S0035-001X200500060000300017&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">18. L.B. Lucy, <i>Astron. J.</i> <b>83</b> (1977) 1013.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315291&pid=S0035-001X200500060000300018&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">19. R.A. Gingold and J.J. Monaghan, <i>Mon. Not. R. Astron. Soc.</i> <b>181</b> (1977) 375.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315293&pid=S0035-001X200500060000300019&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">20. J.J. Monaghan and J.C. Lattanzio, <i>Astron. Astrophys.</i> <b>158</b> (1986) 207.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315295&pid=S0035-001X200500060000300020&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">21. J.C. Lattanzio and R.N. Henriksen, <i>Mon. Not. R. Astron. Soc.</i> <b>232</b> (1988) 565.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315297&pid=S0035-001X200500060000300021&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">22. M.B. Davies, M. Ruffert, W. Benz, and E. Muller, <i>Astron. Astrophys.</i> <b>272</b> (1993) 430.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315299&pid=S0035-001X200500060000300022&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">23. R.S. Klessen, A. Burkert, and M.R. Bate, <i>Astrophys. J.</i> <b>501</b> (1998) L205.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315301&pid=S0035-001X200500060000300023&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">24. S. Kitsionas and A.P. Whitworth, <i>Mon. Not. R. Astron. Soc.</i> <b>330</b> (2002) 129.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315303&pid=S0035-001X200500060000300024&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">25. J.J. Monaghan, <i>J. Comp. Phys.</i> <b>110</b> (1994) 399.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315305&pid=S0035-001X200500060000300025&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">26. O. Kum, W.G. Hoover, and H.A. Posch, <i>Phys. Rev. E</i> <b>52</b> (1995) 4899.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315307&pid=S0035-001X200500060000300026&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">27. S. Nugent and H.A. Posch, <i>Phys. Rev. E.</i> <b>62</b> (2000) 4968.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315309&pid=S0035-001X200500060000300027&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">28. J.J. Monaghan and J.C. Lattanzio, <i>Astron. Astrophys.</i> <b>149</b> (1985) 135.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315311&pid=S0035-001X200500060000300028&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">29. R. W. Hockney and J. W. Eastwood, <i>Computersimulationusing particles,</i> 1st ed. (McGraw&#45;Hill, New York, 1981).    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315313&pid=S0035-001X200500060000300029&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">30. J.J. Monaghan, <i>Proc. Astron. Soc. Australia</i> <b>5</b> (1983) 182.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315315&pid=S0035-001X200500060000300030&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>  	    <!-- ref --><p align="justify"><font face="verdana" size="2">31. J. Barnes and P. Hut, <i>Nature</i> <b>324</b> (1986) 446.    &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=8315317&pid=S0035-001X200500060000300031&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --></font></p>      ]]></body><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ros]]></surname>
<given-names><![CDATA[N.C.J.]]></given-names>
</name>
</person-group>
<source><![CDATA[Appl. Sci. Rev.]]></source>
<year>1960</year>
<volume>9</volume>
<page-range>374</page-range></nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Fortunati]]></surname>
<given-names><![CDATA[F.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Two-phase flow through wellhead chokes]]></article-title>
<source><![CDATA[The SPE-European Spring Meeting 1972 of the Society of Petroleum Engineers of AIME, SPE 3742]]></source>
<year>May </year>
<month>19</month>
<day>72</day>
<page-range>16</page-range><publisher-loc><![CDATA[Amsterdam ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ashford]]></surname>
<given-names><![CDATA[F.E.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Pet. Tech.]]></source>
<year>1974</year>
<month>) </month>
<day>Au</day>
<page-range>843</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[Ashford]]></surname>
<given-names><![CDATA[F.E.]]></given-names>
</name>
<name>
<surname><![CDATA[Pierce]]></surname>
<given-names><![CDATA[P.E.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Pet. Tech.]]></source>
<year>Sept</year>
<month>em</month>
<day>be</day>
<page-range>1145</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abdul-Majeed]]></surname>
<given-names><![CDATA[G.H.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Correlations developed to predict two phase flow through wellhead chokes]]></article-title>
<source><![CDATA[The 1988 Petroleum Society of CIM, Annual Technical Meeting, CIM 88-39-26, Calgary]]></source>
<year>June</year>
<month> 1</month>
<day>98</day>
<page-range>12</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[Perkins]]></surname>
<given-names><![CDATA[T.K.]]></given-names>
</name>
</person-group>
<source><![CDATA[SPE Drilling & Completion]]></source>
<year>Dece</year>
<month>mb</month>
<day>er</day>
<page-range>271</page-range></nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Klapp]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Mendoza]]></surname>
<given-names><![CDATA[G.]]></given-names>
</name>
<name>
<surname><![CDATA[Sigalotti]]></surname>
<given-names><![CDATA[L. Di G.]]></given-names>
</name>
<name>
<surname><![CDATA[Sira]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Numerical simulations of flow through wellhead chokes with the Smoothed Particle Hydrodynamics method]]></article-title>
<source><![CDATA[7th World Conference on Systematics, Cybernetics and Informatics, SCI 2003]]></source>
<year>July</year>
<month> 2</month>
<day>00</day>
<page-range>27</page-range><publisher-loc><![CDATA[Orlando ]]></publisher-loc>
</nlm-citation>
</ref>
<ref id="B8">
<label>8</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hernquist]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[Katz]]></surname>
<given-names><![CDATA[N.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astrophys. J.]]></source>
<year>1989</year>
<volume>70</volume>
<page-range>419</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[Di G. Sigalotti]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[Klapp]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Sira]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[Melean]]></surname>
<given-names><![CDATA[Y.]]></given-names>
</name>
<name>
<surname><![CDATA[Hasmy]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Comp. Phys.]]></source>
<year>2003</year>
<volume>191</volume>
<page-range>622</page-range></nlm-citation>
</ref>
<ref id="B10">
<label>10</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Libersky]]></surname>
<given-names><![CDATA[L.D.]]></given-names>
</name>
<name>
<surname><![CDATA[Petschek]]></surname>
<given-names><![CDATA[A.G.]]></given-names>
</name>
<name>
<surname><![CDATA[Carney]]></surname>
<given-names><![CDATA[T.C.]]></given-names>
</name>
<name>
<surname><![CDATA[Hipp]]></surname>
<given-names><![CDATA[J.R.]]></given-names>
</name>
<name>
<surname><![CDATA[Allahdadi]]></surname>
<given-names><![CDATA[F.A.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Comp. Phys.]]></source>
<year>1993</year>
<volume>109</volume>
<page-range>67</page-range></nlm-citation>
</ref>
<ref id="B11">
<label>11</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Flebbe]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
<name>
<surname><![CDATA[Münzel]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Herold]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Riffert]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Ruder]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astrophys. J.]]></source>
<year>1994</year>
<volume>431</volume>
<page-range>754</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[Watkins]]></surname>
<given-names><![CDATA[S.J.]]></given-names>
</name>
<name>
<surname><![CDATA[Bhattal]]></surname>
<given-names><![CDATA[A.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Francis]]></surname>
<given-names><![CDATA[N.]]></given-names>
</name>
<name>
<surname><![CDATA[Turner]]></surname>
<given-names><![CDATA[J.A.]]></given-names>
</name>
<name>
<surname><![CDATA[Whitworth]]></surname>
<given-names><![CDATA[A.P.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astron. Astrophys. Suppl. Ser.]]></source>
<year>1996</year>
<volume>119</volume>
<page-range>177</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[Morris]]></surname>
<given-names><![CDATA[J.P.]]></given-names>
</name>
<name>
<surname><![CDATA[Fox]]></surname>
<given-names><![CDATA[P.J.]]></given-names>
</name>
<name>
<surname><![CDATA[Zhu]]></surname>
<given-names><![CDATA[Y.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Comp. Phys.]]></source>
<year>1997</year>
<volume>136</volume>
<page-range>214</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[Bonet]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Lok]]></surname>
<given-names><![CDATA[T.-S.L.]]></given-names>
</name>
</person-group>
<source><![CDATA[Comp. Meth. Appl. Mech. Eng.]]></source>
<year>1999</year>
<volume>180</volume>
<page-range>97</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[Sigalotti]]></surname>
<given-names><![CDATA[L.D.]]></given-names>
</name>
<name>
<surname><![CDATA[López]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Donoso]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Sira]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
<name>
<surname><![CDATA[Klapp]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Comp. Phys.]]></source>
<year>2006</year>
<volume>212</volume>
<page-range>124</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[Sigalotti]]></surname>
<given-names><![CDATA[L.D.]]></given-names>
</name>
<name>
<surname><![CDATA[Klapp]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
</person-group>
<source><![CDATA[International Journal of Modern Physics D]]></source>
<year>2001</year>
<volume>10</volume>
<page-range>115</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[Takeda]]></surname>
<given-names><![CDATA[H.]]></given-names>
</name>
<name>
<surname><![CDATA[Miyama]]></surname>
<given-names><![CDATA[S.M.]]></given-names>
</name>
<name>
<surname><![CDATA[Sekiya]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<source><![CDATA[Prog. Theoret. Phys.]]></source>
<year>1994</year>
<volume>92</volume>
<page-range>939</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[Lucy]]></surname>
<given-names><![CDATA[L.B.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astron. J.]]></source>
<year>1977</year>
<volume>83</volume>
<page-range>1013</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[Gingold]]></surname>
<given-names><![CDATA[R.A.]]></given-names>
</name>
<name>
<surname><![CDATA[Monaghan]]></surname>
<given-names><![CDATA[J.J.]]></given-names>
</name>
</person-group>
<source><![CDATA[Mon. Not. R. Astron. Soc.]]></source>
<year>1977</year>
<volume>181</volume>
<page-range>375</page-range></nlm-citation>
</ref>
<ref id="B20">
<label>20</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Monaghan]]></surname>
<given-names><![CDATA[J.J.]]></given-names>
</name>
<name>
<surname><![CDATA[Lattanzio]]></surname>
<given-names><![CDATA[J.C.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astron. Astrophys.]]></source>
<year>1986</year>
<volume>158</volume>
<page-range>207</page-range></nlm-citation>
</ref>
<ref id="B21">
<label>21</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Lattanzio]]></surname>
<given-names><![CDATA[J.C.]]></given-names>
</name>
<name>
<surname><![CDATA[Henriksen]]></surname>
<given-names><![CDATA[R.N.]]></given-names>
</name>
</person-group>
<source><![CDATA[Mon. Not. R. Astron. Soc.]]></source>
<year>1988</year>
<volume>232</volume>
<page-range>565</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[Davies]]></surname>
<given-names><![CDATA[M.B.]]></given-names>
</name>
<name>
<surname><![CDATA[Ruffert]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Benz]]></surname>
<given-names><![CDATA[W.]]></given-names>
</name>
<name>
<surname><![CDATA[Muller]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astron. Astrophys.]]></source>
<year>1993</year>
<volume>272</volume>
<page-range>430</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[Klessen]]></surname>
<given-names><![CDATA[R.S.]]></given-names>
</name>
<name>
<surname><![CDATA[Burkert]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Bate]]></surname>
<given-names><![CDATA[M.R.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astrophys. J.]]></source>
<year>1998</year>
<volume>501</volume>
<page-range>L205</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[Kitsionas]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Whitworth]]></surname>
<given-names><![CDATA[A.P.]]></given-names>
</name>
</person-group>
<source><![CDATA[Mon. Not. R. Astron. Soc.]]></source>
<year>2002</year>
<volume>330</volume>
<page-range>129</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[Monaghan]]></surname>
<given-names><![CDATA[J.J.]]></given-names>
</name>
</person-group>
<source><![CDATA[J. Comp. Phys.]]></source>
<year>1994</year>
<volume>110</volume>
<page-range>399</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[Kum]]></surname>
<given-names><![CDATA[O.]]></given-names>
</name>
<name>
<surname><![CDATA[Hoover]]></surname>
<given-names><![CDATA[W.G.]]></given-names>
</name>
<name>
<surname><![CDATA[Posch]]></surname>
<given-names><![CDATA[H.A.]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rev. E]]></source>
<year>1995</year>
<volume>52</volume>
<page-range>4899</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[Nugent]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Posch]]></surname>
<given-names><![CDATA[H.A.]]></given-names>
</name>
</person-group>
<source><![CDATA[Phys. Rev. E.]]></source>
<year>2000</year>
<volume>62</volume>
<page-range>4968</page-range></nlm-citation>
</ref>
<ref id="B28">
<label>28</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Monaghan]]></surname>
<given-names><![CDATA[J.J.]]></given-names>
</name>
<name>
<surname><![CDATA[Lattanzio]]></surname>
<given-names><![CDATA[J.C.]]></given-names>
</name>
</person-group>
<source><![CDATA[Astron. Astrophys.]]></source>
<year>1985</year>
<volume>149</volume>
<page-range>135</page-range></nlm-citation>
</ref>
<ref id="B29">
<label>29</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hockney]]></surname>
<given-names><![CDATA[R. W.]]></given-names>
</name>
<name>
<surname><![CDATA[Eastwood]]></surname>
<given-names><![CDATA[J. W.]]></given-names>
</name>
</person-group>
<source><![CDATA[Computersimulationusing particles]]></source>
<year>1981</year>
<edition>1</edition>
<publisher-loc><![CDATA[New York ]]></publisher-loc>
<publisher-name><![CDATA[McGraw-Hill]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B30">
<label>30</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Monaghan]]></surname>
<given-names><![CDATA[J.J.]]></given-names>
</name>
</person-group>
<source><![CDATA[Proc. Astron. Soc. Australia]]></source>
<year>1983</year>
<volume>5</volume>
<page-range>182</page-range></nlm-citation>
</ref>
<ref id="B31">
<label>31</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Barnes]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Hut]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
</person-group>
<source><![CDATA[Nature]]></source>
<year>1986</year>
<volume>324</volume>
<page-range>446</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
