Black Hole Supernovae, Their Equation of State Dependence, and Ejecta Composition
Recent literature on core-collapse supernovae suggests that a black hole (BH) can form within ∼1 s of shock revival, while still culminating in a successful supernova. We refer to these as BH supernovae, as they are distinct from other BH formation channels in both timescale and impact on the explos...
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Main Authors: | Oliver Eggenberger Andersen, Evan O’Connor, Haakon Andresen, André da Silva Schneider, Sean M. Couch |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
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Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ada899 |
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