A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory
We describe an asymptotic procedure for deriving continuum equations from the kinetic theory of a simple gas. As in the works of Hilbert, of Chapman and of Enskog, we expand in the mean flight time of the constituent particles of the gas, but we do not adopt the Chapman-Enskog device of simplifying...
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creator | Chen, Xinzhong Rao, Hongling Spiegel, Edward A |
description | We describe an asymptotic procedure for deriving continuum equations from the
kinetic theory of a simple gas. As in the works of Hilbert, of Chapman and of
Enskog, we expand in the mean flight time of the constituent particles of the
gas, but we do not adopt the Chapman-Enskog device of simplifying the formulae
at each order by using results from previous orders. In this way, we are able
to derive a new set of fluid dynamical equations from kinetic theory, as we
illustrate here for the relaxation model for monatomic gases. We obtain a
stress tensor that contains a dynamical pressure term (or bulk viscosity) that
is process-dependent and our heat current depends on the gradients of both
temperature and density. On account of these features, the equations apply to a
greater range of Knudsen number (the ratio of mean free path to macroscopic
scale) than do the Navier-Stokes equations, as we see in the accompanying
paper. In the limit of vanishing Knudsen number, our equations reduce to the
usual Navier-Stokes equations with no bulk viscosity. |
doi_str_mv | 10.48550/arxiv.astro-ph/0105346 |
format | Article |
fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_astro_ph_0105346</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>astro_ph_0105346</sourcerecordid><originalsourceid>FETCH-arxiv_primary_astro_ph_01053463</originalsourceid><addsrcrecordid>eNqNzrEOgjAUQNEuDkb9Bt9iokMRAhhXA6LGzRDXpsESXmJb8lqI_L2G8AFOdznDZWwdhUFyTNNwL-mDfSCdJ8vbZh9GYRonhzl7niCzxqPpOg25chVh69EasDU8JKka1Qsu0kE-GKmxcrC97TjnP0vYy5EWZDXc0SiPFZSNsjQs2ayWb6dWUxdsU5zL7MrHD9ESakmDGH9E24jpJ_7XfQFY6UXh</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory</title><source>arXiv.org</source><creator>Chen, Xinzhong ; Rao, Hongling ; Spiegel, Edward A</creator><creatorcontrib>Chen, Xinzhong ; Rao, Hongling ; Spiegel, Edward A</creatorcontrib><description>We describe an asymptotic procedure for deriving continuum equations from the
kinetic theory of a simple gas. As in the works of Hilbert, of Chapman and of
Enskog, we expand in the mean flight time of the constituent particles of the
gas, but we do not adopt the Chapman-Enskog device of simplifying the formulae
at each order by using results from previous orders. In this way, we are able
to derive a new set of fluid dynamical equations from kinetic theory, as we
illustrate here for the relaxation model for monatomic gases. We obtain a
stress tensor that contains a dynamical pressure term (or bulk viscosity) that
is process-dependent and our heat current depends on the gradients of both
temperature and density. On account of these features, the equations apply to a
greater range of Knudsen number (the ratio of mean free path to macroscopic
scale) than do the Navier-Stokes equations, as we see in the accompanying
paper. In the limit of vanishing Knudsen number, our equations reduce to the
usual Navier-Stokes equations with no bulk viscosity.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0105346</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2001-05</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0105346$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.1103/PhysRevE.64.046308$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0105346$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Chen, Xinzhong</creatorcontrib><creatorcontrib>Rao, Hongling</creatorcontrib><creatorcontrib>Spiegel, Edward A</creatorcontrib><title>A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory</title><description>We describe an asymptotic procedure for deriving continuum equations from the
kinetic theory of a simple gas. As in the works of Hilbert, of Chapman and of
Enskog, we expand in the mean flight time of the constituent particles of the
gas, but we do not adopt the Chapman-Enskog device of simplifying the formulae
at each order by using results from previous orders. In this way, we are able
to derive a new set of fluid dynamical equations from kinetic theory, as we
illustrate here for the relaxation model for monatomic gases. We obtain a
stress tensor that contains a dynamical pressure term (or bulk viscosity) that
is process-dependent and our heat current depends on the gradients of both
temperature and density. On account of these features, the equations apply to a
greater range of Knudsen number (the ratio of mean free path to macroscopic
scale) than do the Navier-Stokes equations, as we see in the accompanying
paper. In the limit of vanishing Knudsen number, our equations reduce to the
usual Navier-Stokes equations with no bulk viscosity.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNqNzrEOgjAUQNEuDkb9Bt9iokMRAhhXA6LGzRDXpsESXmJb8lqI_L2G8AFOdznDZWwdhUFyTNNwL-mDfSCdJ8vbZh9GYRonhzl7niCzxqPpOg25chVh69EasDU8JKka1Qsu0kE-GKmxcrC97TjnP0vYy5EWZDXc0SiPFZSNsjQs2ayWb6dWUxdsU5zL7MrHD9ESakmDGH9E24jpJ_7XfQFY6UXh</recordid><startdate>20010519</startdate><enddate>20010519</enddate><creator>Chen, Xinzhong</creator><creator>Rao, Hongling</creator><creator>Spiegel, Edward A</creator><scope>GOX</scope></search><sort><creationdate>20010519</creationdate><title>A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory</title><author>Chen, Xinzhong ; Rao, Hongling ; Spiegel, Edward A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_astro_ph_01053463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Chen, Xinzhong</creatorcontrib><creatorcontrib>Rao, Hongling</creatorcontrib><creatorcontrib>Spiegel, Edward A</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Chen, Xinzhong</au><au>Rao, Hongling</au><au>Spiegel, Edward A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory</atitle><date>2001-05-19</date><risdate>2001</risdate><abstract>We describe an asymptotic procedure for deriving continuum equations from the
kinetic theory of a simple gas. As in the works of Hilbert, of Chapman and of
Enskog, we expand in the mean flight time of the constituent particles of the
gas, but we do not adopt the Chapman-Enskog device of simplifying the formulae
at each order by using results from previous orders. In this way, we are able
to derive a new set of fluid dynamical equations from kinetic theory, as we
illustrate here for the relaxation model for monatomic gases. We obtain a
stress tensor that contains a dynamical pressure term (or bulk viscosity) that
is process-dependent and our heat current depends on the gradients of both
temperature and density. On account of these features, the equations apply to a
greater range of Knudsen number (the ratio of mean free path to macroscopic
scale) than do the Navier-Stokes equations, as we see in the accompanying
paper. In the limit of vanishing Knudsen number, our equations reduce to the
usual Navier-Stokes equations with no bulk viscosity.</abstract><doi>10.48550/arxiv.astro-ph/0105346</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
title | A Continuum Description of Rarefied Gas Dynamics (I)--- Derivation From Kinetic Theory |
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