The neutrino opacity of neutron rich matter
The study of neutron rich matter, present in neutron star, proto-neutron stars and core-collapse supernovae, can lead to further understanding of the behavior of nuclear matter in highly asymmetric nuclei. Heterogeneous structures are expected to exist in these systems, often referred to as nuclear...
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todo:paper_03759474_v961_n_p183_Alcain2023-10-03T15:30:51Z The neutrino opacity of neutron rich matter Alcain, P.N. Dorso, C.O. Neutrino opacity Neutron rich matter Nuclear equation of state The study of neutron rich matter, present in neutron star, proto-neutron stars and core-collapse supernovae, can lead to further understanding of the behavior of nuclear matter in highly asymmetric nuclei. Heterogeneous structures are expected to exist in these systems, often referred to as nuclear pasta. We have carried out a systematic study of neutrino opacity for different thermodynamic conditions in order to assess the impact that the structure has on it. We studied the dynamics of the neutrino opacity of the heterogeneous matter at different thermodynamic conditions with semiclassical molecular dynamics model already used to study nuclear multifragmentation. For different densities, proton fractions and temperature, we calculate the very long range opacity and the cluster distribution. The neutrino opacity is of crucial importance for the evolution of the core-collapse supernovae and the neutrino scattering. © 2017 Elsevier B.V. Fil:Dorso, C.O. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03759474_v961_n_p183_Alcain |
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Universidad de Buenos Aires |
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I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Neutrino opacity Neutron rich matter Nuclear equation of state |
spellingShingle |
Neutrino opacity Neutron rich matter Nuclear equation of state Alcain, P.N. Dorso, C.O. The neutrino opacity of neutron rich matter |
topic_facet |
Neutrino opacity Neutron rich matter Nuclear equation of state |
description |
The study of neutron rich matter, present in neutron star, proto-neutron stars and core-collapse supernovae, can lead to further understanding of the behavior of nuclear matter in highly asymmetric nuclei. Heterogeneous structures are expected to exist in these systems, often referred to as nuclear pasta. We have carried out a systematic study of neutrino opacity for different thermodynamic conditions in order to assess the impact that the structure has on it. We studied the dynamics of the neutrino opacity of the heterogeneous matter at different thermodynamic conditions with semiclassical molecular dynamics model already used to study nuclear multifragmentation. For different densities, proton fractions and temperature, we calculate the very long range opacity and the cluster distribution. The neutrino opacity is of crucial importance for the evolution of the core-collapse supernovae and the neutrino scattering. © 2017 Elsevier B.V. |
format |
JOUR |
author |
Alcain, P.N. Dorso, C.O. |
author_facet |
Alcain, P.N. Dorso, C.O. |
author_sort |
Alcain, P.N. |
title |
The neutrino opacity of neutron rich matter |
title_short |
The neutrino opacity of neutron rich matter |
title_full |
The neutrino opacity of neutron rich matter |
title_fullStr |
The neutrino opacity of neutron rich matter |
title_full_unstemmed |
The neutrino opacity of neutron rich matter |
title_sort |
neutrino opacity of neutron rich matter |
url |
http://hdl.handle.net/20.500.12110/paper_03759474_v961_n_p183_Alcain |
work_keys_str_mv |
AT alcainpn theneutrinoopacityofneutronrichmatter AT dorsoco theneutrinoopacityofneutronrichmatter AT alcainpn neutrinoopacityofneutronrichmatter AT dorsoco neutrinoopacityofneutronrichmatter |
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1807321802920165376 |