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 \(\sim 1\) s of shock revival, while still culminating in a successful supernova. We refer to these as black hole supernovae, as they are distinct from other BH formation channels in both timescale and impa...
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Veröffentlicht in: | arXiv.org 2024-11 |
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Sprache: | eng |
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