Beta Equilibrium under Neutron Star Merger Conditions
We calculate the nonzero-temperature correction to the beta equilibrium condition in nuclear matter under neutron star merger conditions, in the temperature range 1mEv < <i>T</i> ≲ 5 mEv. We improve on previous work using a consistent description of nuclear matter based on the IUF and...
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| Auteurs principaux: | , , , |
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| Format: | article |
| Langue: | EN |
| Publié: |
MDPI AG
2021
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| Sujets: | |
| Accès en ligne: | https://doaj.org/article/e5dd0214faf3433b83333f2bb21933a0 |
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