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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Autor principal: Dorso, Claudio Oscar
Publicado: 2017
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759474_v961_n_p183_Alcain
http://hdl.handle.net/20.500.12110/paper_03759474_v961_n_p183_Alcain
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spelling paper:paper_03759474_v961_n_p183_Alcain2023-06-08T15:38:23Z The neutrino opacity of neutron rich matter Dorso, Claudio Oscar 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. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759474_v961_n_p183_Alcain 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
Dorso, Claudio Oscar
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.
author Dorso, Claudio Oscar
author_facet Dorso, Claudio Oscar
author_sort Dorso, Claudio Oscar
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
publishDate 2017
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759474_v961_n_p183_Alcain
http://hdl.handle.net/20.500.12110/paper_03759474_v961_n_p183_Alcain
work_keys_str_mv AT dorsoclaudiooscar theneutrinoopacityofneutronrichmatter
AT dorsoclaudiooscar neutrinoopacityofneutronrichmatter
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