110 citations · 411 across the 9 of their papers we have counts for
9 papers
Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model
Masamichi Zaizen, Sherwood Richers, Hiroki Nagakura +2
In the standard model of core-collapse supernova (CCSN), all neutrinos are assumed to be in pure flavor eigenstates in CCSN cores, but the assumption becomes invalid if neutrino di…
A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
S. Furusawa, H. Togashi, H. Nagakura +4
We have constructed a nuclear equation of state (EOS) that includes a full nuclear ensemble for use in core-collapse supernova simulations. It is based on the EOS for uniform nucle…
Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. II. progenitor dependence
K. Sumiyoshi, S. Yamada, H. Suzuki
We study the progenitor dependence of the black hole formation and its associated neutrino signals from the gravitational collapse of non-rotating massive stars, following the prec…
Neutrino signals from the formation of black hole: a probe of equation of state of dense matter
K. Sumiyoshi, S. Yamada, H. Suzuki +1
The gravitational collapse of a non-rotating, black-hole-forming massive star is studied by neutrino-radiation-hydrodynamical simulations for two different sets of realistic equati…
An approach toward the successful supernova explosion by physics of unstable nuclei
K. Sumiyoshi, S. Yamada, H. Suzuki +2
We study the explosion mechanism of collapse-driven supernovae by numerical simulations with a new nuclear EOS based on unstable nuclei. We report new results of simulations of gen…
Properties of a relativistic equation of state for collapse-driven supernovae
K. Sumiyoshi, H. Suzuki, S. Yamada +1
We study characteristics of the relativistic equation of state (EOS) for collapse-driven supernovae, which is derived by relativistic nuclear many body theory. Recently the relativ…