Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics
Ryuichiro Akaho, Hiroki Nagakura, Wakana Iwakami, Shun Furusawa, Akira Harada, Hirotada Okawa, Hideo Matsufuru, Kohsuke Sumiyoshi, and Shoichi Yamada

TL;DR
This study investigates how neutrino fast flavor conversion influences core-collapse supernova explosions, revealing a bifurcated impact depending on progenitor mass and emphasizing the importance of multi-angle neutrino transport modeling.
Contribution
It introduces a multi-angle FFC subgrid model based on quantum kinetic theory and demonstrates its critical role in accurately simulating supernova dynamics.
Findings
FFC facilitates shock revival in low-mass progenitors.
FFC inhibits explosion in higher-mass progenitors.
Mass accretion rate determines FFC's positive or negative impact.
Abstract
In this {\it Letter}, we present a compelling and robust argument for the roles of neutrino fast flavor conversion (FFC) in the explosion mechanism of core-collapse supernova (CCSN), combining the {\it multi-angle} FFC subgrid model rooted in quantum kinetic theory with the multi-dimensional four-species Boltzmann neutrino radiation hydrodynamics. Employing various progenitor masses and the nuclear equations of states, we find that the effect of FFC on CCSN explosion is bifurcated depending on the progenitors. For the lowest-mass progenitor, FFC facilitates the shock revival and enhances the explosion energy, whereas for higher-mass progenitors its impact is inhibitory. We identify the mass accretion rate as the key determinant governing this bifurcation. When the mass accretion rate is low (high), the contribution of FFC to neutrino heating becomes positive (negative), because the…
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