A Parameterized Neutrino Emission Model to Study Mass Ejection in Failed Core-collapse Supernovae

A Parameterized Neutrino Emission Model to Study Mass Ejection in Failed Core-collapse Supernovae

Some massive stars end their lives as failed core-collapse supernovae (CCSNe) and become black holes (BHs). Although in this class of phenomena the stalled supernova (SN) shock is not revived, the outer stellar envelope can still be partially ejected. This occurs because the hydrodynamic equilibrium...

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Bibliographic Details
Main Authors: André da Silva Schneider, Evan O’Connor
Format: Article
Language:English
Published: IOP Publishing 2022-01-01
Series:The Astrophysical Journal
Subjects:
Compact objects
Hydrodynamics
Neutron stars
Core-collapse supernovae
Nuclear astrophysics
Stellar mass black holes
Online Access:https://doi.org/10.3847/1538-4357/aca332

Internet

https://doi.org/10.3847/1538-4357/aca332

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