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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…
Observing Supernova Neutrino Light Curves with Super-Kamiokande. III. Extraction of Mass and Radius of Neutron Stars from Synthetic Data
Yudai Suwa, Akira Harada, Masayuki Harada +6
Neutrinos are guaranteed to be observable from the next galactic supernova (SN). Optical light and gravitational waves are also observable, but may be difficult to observe if the l…
The training response law explains how deep neural networks learn
Kenichi Nakazato
Deep neural network is the widely applied technology in this decade. In spite of the fruitful applications, the mechanism behind that is still to be elucidated. We study the learni…
Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
Yosuke Ashida, Ken'ichiro Nakazato
Core collapse of massive stars leads to different fates for various physical factors, which gives different spectra of the emitted neutrinos. We focus on the supernova relic neutri…