Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics

The Brussels-Montreal equations of state of cold dense nuclear matter that have been recently developed are tested against various constraints coming from both nuclear physics and astrophysics. The nuclear physics constraints include the analysis of nuclear flow and kaon production in heavy-ion coll...

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Main Authors: Fantina A. F., Chamel N., Pearson J. M., Goriely S.
Format: Article
Language:English
Published: EDP Sciences 2014-03-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20146607005
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author Fantina A. F.
Chamel N.
Pearson J. M.
Goriely S.
author_facet Fantina A. F.
Chamel N.
Pearson J. M.
Goriely S.
author_sort Fantina A. F.
collection DOAJ
description The Brussels-Montreal equations of state of cold dense nuclear matter that have been recently developed are tested against various constraints coming from both nuclear physics and astrophysics. The nuclear physics constraints include the analysis of nuclear flow and kaon production in heavy-ion collision experiments, as well as recent microscopic many-body calculations of infinite homogeneous neutron matter. Astrophysical observations, especially recent neutron-star mass measurements, provide valuable constraints on the high-density part of the equation of state that is not accessible in laboratory experiments.
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spelling doaj.art-64f693c503b346699e923b2952f5cb432022-12-21T17:24:02ZengEDP SciencesEPJ Web of Conferences2100-014X2014-03-01660700510.1051/epjconf/20146607005epjconf_inpc2013_07005Constraints on the equation of state of cold dense matter from nuclear physics and astrophysicsFantina A. F.0Chamel N.1Pearson J. M.2Goriely S.3Institut d’Astronomie et d’Astrophysique, CP226, Université Libre de BruxellesInstitut d’Astronomie et d’Astrophysique, CP226, Université Libre de BruxellesDépartement de Physique, Université de MontréalInstitut d’Astronomie et d’Astrophysique, CP226, Université Libre de BruxellesThe Brussels-Montreal equations of state of cold dense nuclear matter that have been recently developed are tested against various constraints coming from both nuclear physics and astrophysics. The nuclear physics constraints include the analysis of nuclear flow and kaon production in heavy-ion collision experiments, as well as recent microscopic many-body calculations of infinite homogeneous neutron matter. Astrophysical observations, especially recent neutron-star mass measurements, provide valuable constraints on the high-density part of the equation of state that is not accessible in laboratory experiments.http://dx.doi.org/10.1051/epjconf/20146607005
spellingShingle Fantina A. F.
Chamel N.
Pearson J. M.
Goriely S.
Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
EPJ Web of Conferences
title Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
title_full Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
title_fullStr Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
title_full_unstemmed Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
title_short Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
title_sort constraints on the equation of state of cold dense matter from nuclear physics and astrophysics
url http://dx.doi.org/10.1051/epjconf/20146607005
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