Direct Monte Carlo simulations of accretion discs

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dc.creatorMatsuda, Takuya
dc.creatorMizutani, Hiromi
dc.creatorBoffin, Henri M. J.
dc.date2001-10-09
dc.date.accessioned2026-07-07T02:00:43Z
dc.date.available2026-07-07T02:00:43Z
dc.descriptionWe apply the Direct Simulation Monte Carlo (DSMC) method, developed originally to calculate rarefied gas dynamical problems, to study the gas flow in an accretion disc in a close binary system. The method involves viscosity and thermal conduction automatically, and can thus simulate turbulent viscosity (alpha viscosity).
dc.description2 pages, 2 figures. To be published in "The Physics of Cataclysmic Variables and Related Objects", ASP Conf. Ser., eds. B. T. Gansicke, K. Beuermann, & K. Reinsch
dc.identifierhttps://arxiv.org/abs/astro-ph/0110199
dc.identifierhttp://arxiv.org/abs/astro-ph/0110199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3502
dc.subjectAstrophysics
dc.titleDirect Monte Carlo simulations of accretion discs
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