NewtonPlus: Approximate Relativity for Supernova Simulations

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dc.creatorCardall, Christian Y.
dc.creatorMezzacappa, Anthony
dc.creatorLiebendoerfer, Matthias
dc.date2001-06-06
dc.date.accessioned2026-07-07T01:58:49Z
dc.date.available2026-07-07T01:58:49Z
dc.descriptionWe propose an approximation to general relativity that captures the main gravitational effects of dynamical importance in supernovae. The conceptual link between this formalism and the Newtonian limit is such that it could likely be implemented in existing multidimensional Newtonian gravitational hydrodynamics codes employing a Poisson solver. As a test of the formalism's utility, we display results for rapidly rotating (and therefore highly deformed) neutron stars.
dc.description20 pages, submitted to Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/astro-ph/0106105
dc.identifierhttp://arxiv.org/abs/astro-ph/0106105
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2868
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNewtonPlus: Approximate Relativity for Supernova Simulations
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