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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 |
| Related resource: | http://dx.doi.org/10.1103/PhysRevC.66.045803 |
| ISSN: | 0556-2813 |
| Appears in Collections: | Articles publicats en revistes (Física Quàntica i Astrofísica) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 508593.pdf | 143.59 kB | Adobe PDF | View/Open |
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