155 citations · 754 across the 16 of their papers we have counts for
16 papers
Detection of the 4.4-MeV gamma rays from O()O(12.97 with a water-Cherenkov detector in the supernova neutrino bursts
Makoto Sakuda, Toshio Suzuki, Mandeep Singh Reen +2
We first discuss and determine the isospin mixing of the two states (12.53 MeV and 12.97 MeV) of O nucleus using the inelastic electron scattering data. We then evalua…
Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling
Kohsuke Sumiyoshi, Shun Furusawa, Hiroki Nagakura +4
We study the influence of hot and dense matter in core-collapse supernovae by adopting up-to-date nuclear equation of state (EOS) based on the microscopic nuclear many-body framewo…
A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos
Ken'ichiro Nakazato, Hideyuki Suzuki
Neutron stars are formed in core-collapse supernova explosions, where a large number of neutrinos are emitted. In this paper, supernova neutrino light curves are computed for the c…
Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations
Kohsuke Sumiyoshi, Ken'ichiro Nakazato, Hideyuki Suzuki +2
We study the influence of density-dependent symmetry energy at high densities in simulations of core-collapse supernovae, black hole formation and proto-neutron star cooling by ext…
Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
Ken'ichiro Nakazato, Hideyuki Suzuki
The cooling process of a protoneutron star is investigated with focus on its sensitivity to properties of hot and dense matter. An equation of state, which includes the nucleon eff…
Heavy Nuclei as Thermal Insulation for Proto-Neutron Stars
Ken'ichiro Nakazato, Hideyuki Suzuki, Hajime Togashi
A proto-neutron star (PNS) is a newly formed compact object in a core collapse supernova. In this Letter, the neutrino emission from the cooling process of a PNS is investigated us…