activity
20052026
most citedThree-dimensional core-collapse supernova simulated using a 15 progenitor

284 citations · 1.3k across the 46 of their papers we have counts for

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Showing 2012Show all

8 papers · 1 filter

astro-ph.SR2012★ 6 cited

Conservative Moment Equations for Neutrino Radiation Transport with Limited Relativity

Eirik Endeve, Christian Y. Cardall, Anthony Mezzacappa

We derive conservative, multidimensional, energy-dependent moment equations for neutrino transport in core-collapse supernovae and related astrophysical systems, with particular at…

astro-ph.SR2012★ 191 cited

Axisymmetric Ab Initio Core-Collapse Supernova Simulations of 12-25 M_sol Stars

Stephen W. Bruenn, Anthony Mezzacappa, W. Raphael Hix +7

We present an overview of four ab initio axisymmetric core-collapse supernova simulations employing detailed spectral neutrino transport computed with our CHIMERA code and initiate…

astro-ph.HE2012★ 82 cited

Conservative 3+1 General Relativistic Variable Eddington Tensor Radiation Transport Equations

Christian Y. Cardall, Eirik Endeve, Anthony Mezzacappa

We present conservative 3+1 general relativistic variable Eddington tensor radiation transport equations, including greater elaboration of the momentum space divergence (that is, t…

astro-ph.IM2012★ 2 cited

GenASiS: General Astrophysical Simulation System. II. Nonrelativistic Hydrodynamics

Christian Y. Cardall, Reuben D. Budiardja, Eirik Endeve +1

In this paper, the second in a series, we document the algorithms and solvers for compressible nonrelativistic hydrodynamics implemented in GenASiS (General Astrophysical Simulatio…

astro-ph.IM2012★ 16 cited

GenASiS: General Astrophysical Simulation System. I. Refinable Mesh and Nonrelativistic Hydrodynamics

Christian Y. Cardall, Reuben D. Budiardja, Eirik Endeve +1

GenASiS (General Astrophysical Simulation System) is a new code being developed initially and primarily, though by no means exclusively, for the simulation of core-collapse superno…

astro-ph.SR2012★ 6 cited

Turbulence and magnetic field amplification from spiral SASI modes in core-collapse supernovae

E. Endeve, C. Y. Cardall, R. D. Budiardja +2

The stationary accretion shock instability (SASI) plays a central role in modern simulations of the explosion phase of core-collapse supernovae (CCSNe). It may be key to realizing…