The equation of state of symmetric and asymmetric nuclear matter

The equation of state (EOS) of nuclear matter is a very important ingredient in the study of nuclear properties, heavy ion collisions, neutron stars and supernova. Accurate assessment of the value of the incompressibility coefficient, K , of symmetric nuclear matter, which is directly related to the...

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Main Author: S. Shlomo
Format: Article
Language:English
Published: Institute for Nuclear Research, National Academy of Sciences of Ukraine 2007-09-01
Series:Ядерна фізика та енергетика
Online Access:http://jnpae.kinr.kiev.ua/21(3)/Articles_PDF/jnpae-2007-3(21)-0007-Shlomo.pdf
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author S. Shlomo
author_facet S. Shlomo
author_sort S. Shlomo
collection DOAJ
description The equation of state (EOS) of nuclear matter is a very important ingredient in the study of nuclear properties, heavy ion collisions, neutron stars and supernova. Accurate assessment of the value of the incompressibility coefficient, K , of symmetric nuclear matter, which is directly related to the curvature of the EOS, is needed to extend our knowledge of the EOS in the vicinity of the saturation point. We review the current status of K as determined from experimental data on isoscalar giant monopole and dipole resonances (compression modes) in nuclei within the microscopic theory of mean-field-based random phase approximation.
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publisher Institute for Nuclear Research, National Academy of Sciences of Ukraine
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series Ядерна фізика та енергетика
spelling doaj-art-39cc37bd5a6f4c0dabbdfe6d492a33c02025-08-20T03:18:46ZengInstitute for Nuclear Research, National Academy of Sciences of UkraineЯдерна фізика та енергетика1818-331X2074-05652007-09-0183(21)716The equation of state of symmetric and asymmetric nuclear matterS. Shlomo0Cyclotron Institute, Texas A&M University, College Station, Texas, USA The equation of state (EOS) of nuclear matter is a very important ingredient in the study of nuclear properties, heavy ion collisions, neutron stars and supernova. Accurate assessment of the value of the incompressibility coefficient, K , of symmetric nuclear matter, which is directly related to the curvature of the EOS, is needed to extend our knowledge of the EOS in the vicinity of the saturation point. We review the current status of K as determined from experimental data on isoscalar giant monopole and dipole resonances (compression modes) in nuclei within the microscopic theory of mean-field-based random phase approximation.http://jnpae.kinr.kiev.ua/21(3)/Articles_PDF/jnpae-2007-3(21)-0007-Shlomo.pdf
spellingShingle S. Shlomo
The equation of state of symmetric and asymmetric nuclear matter
Ядерна фізика та енергетика
title The equation of state of symmetric and asymmetric nuclear matter
title_full The equation of state of symmetric and asymmetric nuclear matter
title_fullStr The equation of state of symmetric and asymmetric nuclear matter
title_full_unstemmed The equation of state of symmetric and asymmetric nuclear matter
title_short The equation of state of symmetric and asymmetric nuclear matter
title_sort equation of state of symmetric and asymmetric nuclear matter
url http://jnpae.kinr.kiev.ua/21(3)/Articles_PDF/jnpae-2007-3(21)-0007-Shlomo.pdf
work_keys_str_mv AT sshlomo theequationofstateofsymmetricandasymmetricnuclearmatter
AT sshlomo equationofstateofsymmetricandasymmetricnuclearmatter