Nuclei beyond the drip line
| Data(s) |
28/01/2010
28/01/2010
2001
|
|---|---|
| Resumo |
In the Thomas-Fermi model, calculations are presented for nuclei beyond the nuclear drip line at zero temperature. These nuclei are in equilibrium by the presence of an external gas, as may be envisaged in the astrophysical scenario. We find that there is a limiting asymmetry beyond which these nuclei can no longer be made stable. |
| Formato |
4 p. application/pdf |
| Identificador |
0556-2813 http://hdl.handle.net/2445/10989 187584 |
| Idioma(s) |
eng |
| Publicador |
The American Physical Society |
| Relação |
Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.64.057306 Physical Review C, 2001, vol. 64, núm. 5, p. 057306-1-057306-4 |
| Direitos |
(c) The American Physical Society, 2001 info:eu-repo/semantics/openAccess |
| Palavras-Chave | #Estructura nuclear #Física nuclear #Nuclear structure #Nuclear physics |
| Tipo |
info:eu-repo/semantics/article |
