Nuclei beyond the drip line

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dc.contributor	Universitat de Barcelona
dc.contributor.author	De, J. N.
dc.contributor.author	Viñas Gausí, Xavier
dc.contributor.author	Patra, S. K.
dc.contributor.author	Centelles Aixalà, Mario
dc.date	2010-01-28T17:01:55Z
dc.date	2010-01-28T17:01:55Z
dc.date	2001
dc.identifier.citation	0556-2813
dc.identifier.citation	187584
dc.identifier.uri	http://hdl.handle.net/2445/10989
dc.format	4 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.64.057306
dc.relation	Physical Review C, 2001, vol. 64, núm. 5, p. 057306-1-057306-4
dc.relation	http://dx.doi.org/10.1103/PhysRevC.64.057306
dc.rights	(c) The American Physical Society, 2001
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	Estructura nuclear
dc.subject	Física nuclear
dc.subject	Nuclear structure
dc.subject	Nuclear physics
dc.title	Nuclei beyond the drip line
dc.type	info:eu-repo/semantics/article
dc.type	info:eu-repo/semantics/publishedVersion
dc.description.abstract	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.