MHD models of stellar core collapse with GenASiS

E. Endeve; C. Y. Cardall; R. D. Budiardja; A. Mezzacappa

doi:10.1088/1742-6596/78/1/012016

MHD models of stellar core collapse with GenASiS

E. Endeve, C. Y. Cardall, R. D. Budiardja, A. Mezzacappa

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Abstract

We present magnetohydrodynamic (MHD) models of stellar core collapse computed with our astrophysical MHD code GenASiS. Microphysics in the models include a realistic equation of state and a simple parametrization of deleptionization during collapse. We give a brief description of some numerical results, and discuss requirements for capturing the physics of the magnetorotational instability in the context of core collapse supernovae.

Original language	English
Article number	012016
Journal	Journal of Physics: Conference Series
Volume	78
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/78/1/012016
State	Published - Jul 1 2007

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10.1088/1742-6596/78/1/012016

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title = "MHD models of stellar core collapse with GenASiS",

abstract = "We present magnetohydrodynamic (MHD) models of stellar core collapse computed with our astrophysical MHD code GenASiS. Microphysics in the models include a realistic equation of state and a simple parametrization of deleptionization during collapse. We give a brief description of some numerical results, and discuss requirements for capturing the physics of the magnetorotational instability in the context of core collapse supernovae.",

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AU - Mezzacappa, A.

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N2 - We present magnetohydrodynamic (MHD) models of stellar core collapse computed with our astrophysical MHD code GenASiS. Microphysics in the models include a realistic equation of state and a simple parametrization of deleptionization during collapse. We give a brief description of some numerical results, and discuss requirements for capturing the physics of the magnetorotational instability in the context of core collapse supernovae.

AB - We present magnetohydrodynamic (MHD) models of stellar core collapse computed with our astrophysical MHD code GenASiS. Microphysics in the models include a realistic equation of state and a simple parametrization of deleptionization during collapse. We give a brief description of some numerical results, and discuss requirements for capturing the physics of the magnetorotational instability in the context of core collapse supernovae.

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MHD models of stellar core collapse with GenASiS

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