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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Autores principales: Alcain, P.N., Dorso, C.O.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03759474_v961_n_p183_Alcain
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spelling 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
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection 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
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