activity
20242026
collaborators

9 papers

astro-ph.HE2026

Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems

Shota Takahashi, Hiroki Nagakura, Masamichi Zaizen +2

Neutrino flavor evolution in dense astrophysical environments such as core-collapse supernova (CCSN) is influenced by collective effects. While the Fast Flavor Instability (FFI) an…

astro-ph.HE2026

Fast Neutrino-Flavor Conversion with Attenuation and Global Lepton Gradient

Masamichi Zaizen, Hiroki Nagakura

Fast neutrino-flavor conversion (FFC) can nontrivially alter neutrino radiation field in core-collapase supernovae (CCSN) and binary neutron-star merger (BNSM) remnants. However, i…

astro-ph.HE2025

Neutrino Constraints on Black Hole Formation in M31

Yudai Suwa, Ryuichiro Akaho, Yosuke Ashida +9

We investigate neutrino signals associated with black hole formation resulting from the gravitational collapse of massive stars, motivated by the candidate failed supernova M31-201…

astro-ph.HE2025

Dynamical equilibria of fast neutrino flavor conversion

Jiabao Liu, Lucas Johns, Hiroki Nagakura +2

Dense neutrino systems, which display collectivity mediated by the weak interaction, have deep parallels with mean-field kinetic systems governed by other fundamental forces. We id…

astro-ph.HE2025

Observing Supernova Neutrino Light Curves with Super-Kamiokande.VI. A Practical Data Analysis Technique Considering Realistic Experimental Backgrounds

Fumi Nakanishi, Ken'ichiro Nakazato, Masayuki Harada +9

Neutrinos from supernovae, especially those emitted during the late phase of core collapse, are essential for understanding the final stages of massive star evolution. We have been…

hep-ph2025

Spectral diversity in collisional neutrino-flavor conversion: flavor equipartition or swap

Masamichi Zaizen

Quantum kinetics of neutrinos are known to potentially change the classical neutrino radiation field in high-energy astrophysical sources such as core-collapse supernovae and binar…