Nuclei beyond the drip line

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In 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.
Physical Review C (in press), 1 ReVteX file for text, 4 PS-files for figures

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Nuclear Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/218739

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/nucl-th/0108071
 http://arxiv.org/abs/nucl-th/0108071
 Phys.Rev.C64:057306,2001
 doi:10.1103/PhysRevC.64.057306

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arXiv