| HAL : hal-00119539, version 2 |
| arXiv : nucl-th/0612044 |
| Fiche détaillée | Récupérer au format |
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| Nuclear Physics A 789 (2007) 403-425 |
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| Versions disponibles : | v1 (11-12-2006) | v2 (19-04-2007) |
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| Isospin-dependent clusterization of Neutron-Star Matter |
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| C. Ducoin1, 2Philippe Chomaz1F. Gulminelli2 |
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| (01/06/2007) |
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| Because of the presence of a liquid-gas phase transition in nuclear matter, compact-star matter can present a region of instability against the formation of clusters. We investigate this phase separation in a matter composed of neutrons, protons and electrons, within a Skyrme-Lyon mean-field approach. Matter instability and phase properties are characterized through the study of the free-energy curvature. The effect of beta-equilibrium is also analyzed in detail, and we show that the opacity to neutrinos has an influence on the presence of clusterized matter in finite-temperature proto-neutron stars. |
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| 1 : | GANIL - Grand Accélérateur National d'Ions Lourds |
| 2 : | LPCC - Laboratoire de Physique Corpusculaire de Caen |
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| Physique théorique |
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| Domaine | : | Physique/Physique Nucléaire Théorique Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique |
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| nuclear matter – star matter – liquid-gas phase transition – matter clusterization |
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| Liste des fichiers attachés à ce document : | ||||||||||
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| hal-00119539, version 2 | |
| http://hal.archives-ouvertes.fr/hal-00119539 | |
| oai:hal.archives-ouvertes.fr:hal-00119539 | |
| Contributeur : Camille Ducoin | |
| Soumis le : Jeudi 19 Avril 2007, 17:47:47 | |
| Dernière modification le : Lundi 4 Juin 2007, 09:42:36 | |