Fragmentation and clustering in star matter
The specificity of the crust-core phase transition in neutron star at zero and finite temperature will be discussed. It will be shown that, as a consequence of the presence of long range Coulomb interactions, the equivalence of statistical ensembles is violated and a clusterised phase is expected wh...
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EDP Sciences
2012-07-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20123100018 |
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doaj-81c10e96828a45a6afaa6c964591193c2021-08-02T09:35:14ZengEDP SciencesEPJ Web of Conferences2100-014X2012-07-01310001810.1051/epjconf/20123100018Fragmentation and clustering in star matterGulminelli F.The specificity of the crust-core phase transition in neutron star at zero and finite temperature will be discussed. It will be shown that, as a consequence of the presence of long range Coulomb interactions, the equivalence of statistical ensembles is violated and a clusterised phase is expected which is not accessible in the grancanonical ensemble. A specific analytical Nuclear Statistical Equilibrium model will be presented and some new quantitative results relevant for the supernova dynamics will be shown. Finally, the analogies and differences with the phenomenon of nuclear fragmentation will be highlighted. http://dx.doi.org/10.1051/epjconf/20123100018 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Gulminelli F. |
spellingShingle |
Gulminelli F. Fragmentation and clustering in star matter EPJ Web of Conferences |
author_facet |
Gulminelli F. |
author_sort |
Gulminelli F. |
title |
Fragmentation and clustering in star matter |
title_short |
Fragmentation and clustering in star matter |
title_full |
Fragmentation and clustering in star matter |
title_fullStr |
Fragmentation and clustering in star matter |
title_full_unstemmed |
Fragmentation and clustering in star matter |
title_sort |
fragmentation and clustering in star matter |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2012-07-01 |
description |
The specificity of the crust-core phase transition in neutron star at zero and finite temperature will be discussed. It will be shown that, as a consequence of the presence of long range Coulomb interactions, the equivalence of statistical ensembles is violated and a clusterised phase is expected which is not accessible in the grancanonical ensemble. A specific analytical Nuclear Statistical Equilibrium model will be presented and some new quantitative results relevant for the supernova dynamics will be shown. Finally, the analogies and differences with the phenomenon of nuclear fragmentation will be highlighted. |
url |
http://dx.doi.org/10.1051/epjconf/20123100018 |
work_keys_str_mv |
AT gulminellif fragmentationandclusteringinstarmatter |
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