Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach


Autoria(s): Barranco Gómez, Manuel; Buchler, Jean-Robert
Contribuinte(s)

Universitat de Barcelona

Data(s)

04/05/2010

Resumo

The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model.

Identificador

http://hdl.handle.net/2445/12235

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