activity
20242026
collaborators

5 papers

astro-ph.HE2026

Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase

Chinami Kato, Hiroki Nagakura, Akira Ito +4

We present the first systematic study of neutrino emissions from massive stars, continuously tracking the late evolutionary stages through the early core-collapse supernova phase.…

astro-ph.HE2025

Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae

Ryota Hatami, Nozomu Tominaga, Takashi Yoshida +2

We present the results of simulations of nucleosynthesis in a core-collapse supernova (CCSN) including the neutrino process. Using the Si layer of zero-metal progenitor…

astro-ph.HE2025

Extreme anisotropies in deep layers of an exploding star: overabundance of Cr in the northeastern jet of Cassiopeia A

Vincenzo Sapienza, Marco Miceli, Masaomi Ono +5

Core-collapse supernovae drive nucleosynthesis under extreme thermodynamic conditions, and complex mechanisms are at work prompting the transport of heavy elements from deep stella…

astro-ph.HE2025

Inhomogeneous stellar mixing in the final hours before the Cassiopeia A supernova

Toshiki Sato, Kai Matsunaga, Hiroyuki Uchida +10

Understanding stars and their evolution is a key goal of astronomical research and has long been a focus of human interest. In recent years, theorists have paid much attention to t…

astro-ph.HE2024

Evidence for Type Ib/c origin of the supernova remnant G292.0+1.8

Takuto Narita, Hiroyuki Uchida, Jacco Vink +6

Circumstellar material (CSM) produced by mass loss from massive stars () through strong stellar winds or binary stripping provides rich information for underst…