activity
20172026
most citedImaging the Schwarzschild-radius-scale Structure of M87 with the Event Horizon Telescope using Sparse Modeling

178 citations · 726 across the 27 of their papers we have counts for

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Showing astro-ph.HEShow all

23 papers · 1 filter

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

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…

astro-ph.HE2025★ 2 cited

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★ 16 cited

Asymptotic states of fast neutrino-flavor conversions in the three-flavor framework

Jiabao Liu, Hiroki Nagakura, Masamichi Zaizen +2

There has been growing evidence that mu and tau neutrinos are noticeably different due to the emergence of muons in core-collapse supernovae (CCSNe) and binary neutron star mergers…

astro-ph.HE2025

Resolution requirements for numerical modeling of neutrino quantum kinetics

Hiroki Nagakura, Masamichi Zaizen, Jiabao Liu +1

Neutrino quantum kinetics is a rapidly evolving field in computational astrophysics, with a primary focus on collective neutrino oscillations in core-collapse supernovae and post-m…

astro-ph.HE2024★ 11 cited

Quasi-steady evolution of fast neutrino-flavor conversions

Jiabao Liu, Hiroki Nagakura, Masamichi Zaizen +3

In astrophysical environments such as core-collapse supernovae (CCSNe) and binary neutron star mergers (BNSMs), neutrinos potentially experience substantial flavor mixing due to th…

astro-ph.HE2024

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…

astro-ph.HE2023★ 1 cited

BGK subgrid model for neutrino quantum kinetics

Hiroki Nagakura, Lucas Johns, Masamichi Zaizen

We present a new subgrid model for neutrino quantum kinetics, which is primarily designed to incorporate effects of collective neutrino oscillations into neutrino-radiation-hydrody…

astro-ph.HE2023★ 36 cited

Universality of the Neutrino Collisional Flavor Instability in Core Collapse Supernovae

Jiabao Liu, Hiroki Nagakura, Ryuichiro Akaho +3

Neutrinos are known to undergo flavor conversion processes among the three flavors. The fast flavor conversion (FFC) has been the central piece of flavor conversions taking place i…

astro-ph.HE2023★ 13 cited

Fast neutrino-flavor swap in high-energy astrophysical environments

Masamichi Zaizen, Hiroki Nagakura

We assert that non-linear features of fast neutrino-flavor conversion (FFC) can be qualitatively different between core-collapse supernovae (CCSNe) and binary neutron star mergers…

astro-ph.HE2023★ 40 cited

Collisional and Fast Neutrino Flavor Instabilities in Two-dimensional Core-collapse Supernova Simulation with Boltzmann Neutrino Transport

Ryuichiro Akaho, Jiabao Liu, Hiroki Nagakura +2

We present a comprehensive study on the occurrences of the collisional flavor instability (CFI) and the fast flavor instability (FFI) of neutrinos based on a two-dimensional (2D) c…

astro-ph.HE2023

Basic characteristics of neutrino flavor conversions in the post-shock regions of core-collapse supernova

Hiroki Nagakura, Masamichi Zaizen

One of the active debates in core-collapse supernova (CCSN) theory is how significantly neutrino flavor conversions induced by neutrino-neutrino self-interactions change the conven…

astro-ph.HE2023★ 51 cited

Characterizing quasi-steady states of fast neutrino-flavor conversion by stability and conservation laws

Masamichi Zaizen, Hiroki Nagakura

The question of what ingredients characterize the quasi-steady state of fast neutrino-flavor conversion (FFC) is one of the long-standing riddles in neutrino oscillation. Addressin…

astro-ph.HE2023★ 15 cited

Flavor conversions with energy-dependent neutrino emission and absorption

Chinami Kato, Hiroki Nagakura, Masamichi Zaizen

Fast neutrino flavor conversions (FFCs) and collisional flavor instabilities (CFIs) potentially affect the dynamics of core-collapse supernovae (CCSNe) and binary neutron star merg…

astro-ph.HE2022★ 71 cited

Simple method for determining asymptotic states of fast neutrino-flavor conversion

Masamichi Zaizen, Hiroki Nagakura

Neutrino-neutrino forward scatterings potentially induce collective neutrino oscillation in dense neutrino gases in astrophysical sites such as core-collapse supernovae (CCSN) and…

astro-ph.HE2022★ 35 cited

Connecting small-scale to large-scale structures of fast neutrino-flavor conversion

Hiroki Nagakura, Masamichi Zaizen

We present a systematic study of fast neutrino-flavor conversion (FFC) with both small-scale and large-scale numerical simulations in spherical symmetry. We find that FFCs can, in…

astro-ph.HE2022★ 77 cited

Time-dependent and quasi-steady features of fast neutrino-flavor conversion

Hiroki Nagakura, Masamichi Zaizen

Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs in core-collapse supernova and binary neutron star merger, the lack of global simu…

astro-ph.HE2022★ 64 cited

Code Comparison for Fast Flavor Instability Simulation

Sherwood Richers, Huaiyu Duan, Meng-Ru Wu +5

The fast flavor instability (FFI) is expected to be ubiquitous in core-collapse supernovae and neutron star mergers. It rapidly shuffles neutrino flavor in a way that could impact…

astro-ph.HE2020★ 14 cited

Three-flavor collective neutrino conversions with multi-azimuthal-angle instability in an electron-capture supernova model

Masamichi Zaizen, Shunsaku Horiuchi, Tomoya Takiwaki +4

We investigate the multi-azimuthal angle (MAA) effect on collective neutrino oscillation by considering the three-dimensional neutrino momentum distribution in a realistic electron…

astro-ph.HE2019★ 32 cited

Neutrino halo effect on collective neutrino oscillation in iron core-collapse supernova model of a 9.6 star

Masamichi Zaizen, John F. Cherry, Tomoya Takiwaki +4

We extend the multi-angle computational framework and investigate the time evolution of the neutrino halo on collective neutrino oscillation in the core collapse of an iron core pr…

astro-ph.HE2018★ 13 cited

Collective neutrino oscillations and detectabilities in failed supernovae

Masamichi Zaizen, Takashi Yoshida, Kohsuke Sumiyoshi +1

We investigate the collective neutrino oscillations under the three flavor multi-angle approximation in a spherically symmetric simulation of failed supernovae. A failed supernova…