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dc.contributor | Universitat de Barcelona |
---|---|
dc.contributor.author | Barranco Gómez, Manuel |
dc.contributor.author | Buchler, Jean-Robert |
dc.date | 2010-04-22T11:56:21Z |
dc.date | 2010-04-22T11:56:21Z |
dc.date | 1981 |
dc.identifier.citation | 0556-2813 |
dc.identifier.citation | 75989 |
dc.identifier.uri | http://hdl.handle.net/2445/12235 |
dc.format | 12 p. |
dc.format | application/pdf |
dc.language.iso | eng |
dc.publisher | The American Physical Society |
dc.relation | Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.24.1191 |
dc.relation | Physical Review C, 1981, vol. 24, núm. 3, p. 1191-1202 |
dc.relation | http://dx.doi.org/10.1103/PhysRevC.24.1191 |
dc.rights | (c) The American Physical Society, 1981 |
dc.rights | info:eu-repo/semantics/openAccess |
dc.subject | Estructura nuclear |
dc.subject | Astrofísica nuclear |
dc.subject | Ecuacions d'estat |
dc.subject | Nuclear structure |
dc.subject | Nuclear astrophysics |
dc.subject | Equations of state |
dc.title | Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach |
dc.type | info:eu-repo/semantics/article |
dc.type | info:eu-repo/semantics/publishedVersion |
dc.description.abstract |