Isospin-rich nuclei in neutron star matter

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 eme...

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Detalles Bibliográficos
Autores: Sil, Tapas, Samaddar, S. K., Viñas Gausí, Xavier, Centelles Aixalà, Mario, Agrawal, B. K., Patra, S. K.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2002
País:España
Institución:Universidad de Barcelona
Repositorio:Dipòsit Digital de la UB
OAI Identifier:oai:diposit.ub.edu:2445/11001
Acceso en línea:https://hdl.handle.net/2445/11001
Access Level:acceso abierto
Palabra clave:Astrofísica nuclear
Estructura nuclear
Nuclear astrophysics
Nuclear structure
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spelling Isospin-rich nuclei in neutron star matterSil, TapasSamaddar, S. K.Viñas Gausí, XavierCentelles Aixalà, MarioAgrawal, B. K.Patra, S. K.Astrofísica nuclearEstructura nuclearNuclear astrophysicsNuclear structureStability 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.The American Physical Society2002info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionapplication/pdfhttps://hdl.handle.net/2445/11001Articles publicats en revistes (Física Quàntica i Astrofísica)reponame:Dipòsit Digital de la UBinstname:Universidad de BarcelonaInglésReproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.66.045803Physical Review C, 2002, vol. 66, núm. 4, p. 045803-1-045803-9http://dx.doi.org/10.1103/PhysRevC.66.045803(c) The American Physical Society, 2002info:eu-repo/semantics/openAccessoai:diposit.ub.edu:2445/110012026-05-27T06:46:51Z
dc.title.none.fl_str_mv Isospin-rich nuclei in neutron star matter
title Isospin-rich nuclei in neutron star matter
spellingShingle Isospin-rich nuclei in neutron star matter
Sil, Tapas
Astrofísica nuclear
Estructura nuclear
Nuclear astrophysics
Nuclear structure
title_short Isospin-rich nuclei in neutron star matter
title_full Isospin-rich nuclei in neutron star matter
title_fullStr Isospin-rich nuclei in neutron star matter
title_full_unstemmed Isospin-rich nuclei in neutron star matter
title_sort Isospin-rich nuclei in neutron star matter
dc.creator.none.fl_str_mv Sil, Tapas
Samaddar, S. K.
Viñas Gausí, Xavier
Centelles Aixalà, Mario
Agrawal, B. K.
Patra, S. K.
author Sil, Tapas
author_facet Sil, Tapas
Samaddar, S. K.
Viñas Gausí, Xavier
Centelles Aixalà, Mario
Agrawal, B. K.
Patra, S. K.
author_role author
author2 Samaddar, S. K.
Viñas Gausí, Xavier
Centelles Aixalà, Mario
Agrawal, B. K.
Patra, S. K.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Astrofísica nuclear
Estructura nuclear
Nuclear astrophysics
Nuclear structure
topic Astrofísica nuclear
Estructura nuclear
Nuclear astrophysics
Nuclear structure
description 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.
publishDate 2002
dc.date.none.fl_str_mv 2002
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://hdl.handle.net/2445/11001
url https://hdl.handle.net/2445/11001
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.66.045803
Physical Review C, 2002, vol. 66, núm. 4, p. 045803-1-045803-9
http://dx.doi.org/10.1103/PhysRevC.66.045803
dc.rights.none.fl_str_mv (c) The American Physical Society, 2002
info:eu-repo/semantics/openAccess
rights_invalid_str_mv (c) The American Physical Society, 2002
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv The American Physical Society
publisher.none.fl_str_mv The American Physical Society
dc.source.none.fl_str_mv Articles publicats en revistes (Física Quàntica i Astrofísica)
reponame:Dipòsit Digital de la UB
instname:Universidad de Barcelona
instname_str Universidad de Barcelona
reponame_str Dipòsit Digital de la UB
collection Dipòsit Digital de la UB
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15,300719

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