Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach
Contribuinte(s) |
Universitat de Barcelona |
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Data(s) |
04/05/2010
|
Resumo |
The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model. |
Identificador | |
Idioma(s) |
eng |
Publicador |
The American Physical Society |
Direitos |
(c) The American Physical Society, 1981 info:eu-repo/semantics/openAccess |
Palavras-Chave | #Estructura nuclear #Astrofísica nuclear #Ecuacions d'estat #Nuclear structure #Nuclear astrophysics #Equations of state |
Tipo |
info:eu-repo/semantics/article |