Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/11001
Title: Isospin-rich nuclei in neutron star matter
Author: Sil, Tapas
Samaddar, S. K.
Viñas Gausí, Xavier
Centelles Aixalà, Mario
Agrawal, B. K.
Patra, S. K.
Keywords: Astrofísica nuclear
Estructura nuclear
Nuclear astrophysics
Nuclear structure
Issue Date: 2002
Publisher: The American Physical Society
Abstract: Stability of nuclei beyond the drip lines in the presence of an enveloping gas of nucleons and electrons, as prevailing in the inner crust of a neutron star, is studied in the temperature-dependent Thomas-Fermi framework. A limiting asymmetry in the isospin space beyond which nuclei cannot exist emerges from the calculations. The ambient conditions such as temperature, baryon density, and neutrino concentration under which these exotic nuclear systems can be formed are studied in some detail.
Note: Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.66.045803
It is part of: Physical Review C, 2002, vol. 66, núm. 4, p. 045803-1-045803-9
URI: http://hdl.handle.net/2445/11001
ISSN: 0556-2813
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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