Add to ORKGBased on general relativistic three-flavor Boltzmann neutrino transport, we compare simulations of the postbounce evolution for five different stellar progenitors with 13 and 20 solar masses (Nomoto & Hashimoto '88), and 15, 25, and 40 solar masses (Woosley & Weaver '95)
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interacti...
The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neut...
20 pages, 21 figures. Minor revisions. Accepted for publication in ApJ. A version with high-resoluti...
We perform spherically symmetric general-relativistic simulations of core collapse and the postbounc...
In spherical symmetry, very reliable models of stellar core collapse, bounce, and the postbounce pha...
We compare Newtonian three-flavor multigroup Boltzmann (MGBT) and (Bruenn's) multigroup flux-limited...
We have developed a new implicit, multi-group, time-dependent, spherical neutrino transport algorith...
In this paper, we present results from a simulation of stellar core collapse, bounce, and postbounce...
AbstractCore collapse supernovae occupy a special place in the cosmic hierarchy for their role in di...
We present results from dynamical models of core-collapse supernovae in one spatial dimension, emplo...
We investigate the behavior and consequences of the reverse shock that terminates the supersonic exp...
A nascent neutron star resulting from stellar collapse is a prodigious source of neutrinos of all fl...
Core-collapse supernovae are, despite their spectacular visual display, neutrino events. Virtually a...
We present here the first results of two-dimensional hydrodynamical simulations of the neutrino-heat...
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interacti...
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interacti...
The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neut...
20 pages, 21 figures. Minor revisions. Accepted for publication in ApJ. A version with high-resoluti...
We perform spherically symmetric general-relativistic simulations of core collapse and the postbounc...
In spherical symmetry, very reliable models of stellar core collapse, bounce, and the postbounce pha...
We compare Newtonian three-flavor multigroup Boltzmann (MGBT) and (Bruenn's) multigroup flux-limited...
We have developed a new implicit, multi-group, time-dependent, spherical neutrino transport algorith...
In this paper, we present results from a simulation of stellar core collapse, bounce, and postbounce...
AbstractCore collapse supernovae occupy a special place in the cosmic hierarchy for their role in di...
We present results from dynamical models of core-collapse supernovae in one spatial dimension, emplo...
We investigate the behavior and consequences of the reverse shock that terminates the supersonic exp...
A nascent neutron star resulting from stellar collapse is a prodigious source of neutrinos of all fl...
Core-collapse supernovae are, despite their spectacular visual display, neutrino events. Virtually a...
We present here the first results of two-dimensional hydrodynamical simulations of the neutrino-heat...
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interacti...
We explore the effects of collective neutrino flavor oscillations due to neutrino-neutrino interacti...
The mechanism driving core-collapse supernovae is sensitive to the interplay between matter and neut...
20 pages, 21 figures. Minor revisions. Accepted for publication in ApJ. A version with high-resoluti...