Nuclei beyond the drip line

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dc.creatorDe, J. N.
dc.creatorViñas, X.
dc.creatorPatra, S. K.
dc.creatorCentelles, M.
dc.date2001-08-31
dc.date.accessioned2026-07-07T12:38:22Z
dc.date.available2026-07-07T12:38:22Z
dc.descriptionIn a 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.
dc.descriptionPhysical Review C (in press), 1 ReVteX file for text, 4 PS-files for figures
dc.identifierhttps://arxiv.org/abs/nucl-th/0108071
dc.identifierhttp://arxiv.org/abs/nucl-th/0108071
dc.identifierPhys.Rev.C64:057306,2001
dc.identifierdoi:10.1103/PhysRevC.64.057306
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218739
dc.subjectNuclear Theory
dc.titleNuclei beyond the drip line
dc.typetext

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