Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects
Kohsuke Sumiyoshi, Hajime Togashi, Shun Furusawa, Shuying Li, Hong Shen, Ken'ichiro Nakazato, Hideyuki Suzuki
astro-ph.HE, nucl-th
Submitted: 2026-08-06
Comments: 27 pages, 11 figures, submitted to PRC
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Equations of state for supernovae and compact stars
- Equation of state in neutron stars and supernovae
- Explosion Mechanisms of Core-Collapse Supernovae
- Perspectives on Core-Collapse Supernova Theory
- Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae
- Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview
- Long-Term Multidimensional Models of Core-Collapse Supernovae: Progress and Challenges
- Dynamics and Equation of State Dependencies of Relevance for Nucleosynthesis in Supernovae and Neutron Star Mergers
- Neutron Stars and the Nuclear Equation of State
- Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations
- Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
- Supernova Neutrinos: Production, Oscillations and Detection
- Neutrino Emission as Diagnostics of Core-Collapse Supernovae
- Gravitational Waves from Core-Collapse Supernovae
- Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling
- Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature
- Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state
- Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase
- Core-collapse supernova equations of state based on neutron star observations
- Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae
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