Equation of State effects in Core-Collapse Supernovae
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The state of matter at extreme densities remains highly uncertain. Exploding stars provide the extraordinary conditions necessary to access this fascinating high-energy regime. Throughout this thesis, we will review and analyse methods for using the Core-Collapse Supernova mechanism as a future laboratory to study matter at and above multiple times nuclear saturation density.
创建时间：
2024-02-07
