Influence of Effective Nucleon Mass on Equation of State for Supernova Simulations and Neutron Stars

Influence of Effective Nucleon Mass on Equation of State for Supernova Simulations and Neutron Stars

We investigate the influence of the effective nucleon mass on the equation of state (EOS), which is constructed for simulations of core-collapse supernovae and binary neutron star mergers, within the relativistic mean-field (RMF) framework. The study introduces a new RMF parameter set, TM1m, which i...

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Bibliographic Details
Main Authors: Shuying Li, Junbo Pang, Hong Shen, Jinniu Hu, Kohsuke Sumiyoshi
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Core-collapse supernovae
Neutron stars
Online Access:https://doi.org/10.3847/1538-4357/ada6b3
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