Simulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport

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dc.creatorMezzacappa, Anthony
dc.date1997-04-17
dc.date.accessioned2026-07-07T02:23:14Z
dc.date.available2026-07-07T02:23:14Z
dc.descriptionIn one dimension, we present results from comparisons of stationary state multigroup flux-limited diffusion and Boltzmann neutrino transport, focusing on quantities central to the postbounce shock reheating. In two dimensions, we present results from simulations that couple one-dimensional multigroup flux-limited diffusion to two-dimensional PPM hydrodynamics.
dc.descriptionLatex, using sprocl.sty, 3 pages, To appear in the proceedings of the 18th Texas Symposium on Relativistic Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/9704181
dc.identifierhttp://arxiv.org/abs/astro-ph/9704181
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11174
dc.subjectAstrophysics
dc.titleSimulations of Core Collapse Supernovae In One and Two Dimemsions Using Multigroup Neutrino Transport
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