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...
Guardado en:
Autores principales: | , , , |
---|---|
Formato: | article |
Lenguaje: | EN |
Publicado: |
MDPI AG
2021
|
Materias: | |
Acceso en línea: | https://doaj.org/article/e5dd0214faf3433b83333f2bb21933a0 |
Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|