Collective features of nuclear dynamics with exotic nuclei within microscopic transport models
We employ a transport model based on Landau-Vlasov equation to explore the dipolar response of neutron rich systems and its dependence on the symmetry energy. We present evidences for collective features of the Pygmy Dipole Resonance (PDR) and study its dependence with the mass number. We extract a...
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2014-03-01
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Online Access: | http://dx.doi.org/10.1051/epjconf/20146603004 |
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doaj-7d4d0a1455b845f09b27849a8993d6992021-08-02T15:59:29ZengEDP SciencesEPJ Web of Conferences2100-014X2014-03-01660300410.1051/epjconf/20146603004epjconf_inpc2013_03004Collective features of nuclear dynamics with exotic nuclei within microscopic transport modelsBaran Virgil0Colonna Maria1Di Toro MassimoCroitoru Andreea2Dumitru Daniel3Faculty of Physics, University of BucharestLaboratori Nazionali del Sud, INFNFaculty of Physics, University of BucharestFaculty of Physics, University of Bucharest We employ a transport model based on Landau-Vlasov equation to explore the dipolar response of neutron rich systems and its dependence on the symmetry energy. We present evidences for collective features of the Pygmy Dipole Resonance (PDR) and study its dependence with the mass number. We extract a parametrization for the energy centroid position, 41A−1/3, which agrees quite well with the data for Ni, Zr, Sn and Pb. A linear correlation between the Energy Weighted Sum Rule (EWSR) associated to PDR and the neutron skin thickness is evidenced. An increase of 15 MeV fm2 of EWSR to a change of 0.1 fm of neutron skin size is obtained. We conclude that different nuclei having close neutron skin size will exhaust the same EWSR in the pygmy region. Consequently a precise experimental estimate of total EWSR exhausted by PDR allows the determination of the neutron skin size and to constrain the slope parameter of the symmetry energy. http://dx.doi.org/10.1051/epjconf/20146603004 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Baran Virgil Colonna Maria Di Toro Massimo Croitoru Andreea Dumitru Daniel |
spellingShingle |
Baran Virgil Colonna Maria Di Toro Massimo Croitoru Andreea Dumitru Daniel Collective features of nuclear dynamics with exotic nuclei within microscopic transport models EPJ Web of Conferences |
author_facet |
Baran Virgil Colonna Maria Di Toro Massimo Croitoru Andreea Dumitru Daniel |
author_sort |
Baran Virgil |
title |
Collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
title_short |
Collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
title_full |
Collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
title_fullStr |
Collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
title_full_unstemmed |
Collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
title_sort |
collective features of nuclear dynamics with exotic nuclei within microscopic transport models |
publisher |
EDP Sciences |
series |
EPJ Web of Conferences |
issn |
2100-014X |
publishDate |
2014-03-01 |
description |
We employ a transport model based on Landau-Vlasov equation to explore the dipolar response of neutron rich systems and its dependence on the symmetry energy. We present evidences for collective features of the Pygmy Dipole Resonance (PDR) and study its dependence with the mass number. We extract a parametrization for the energy centroid position, 41A−1/3, which agrees quite well with the data for Ni, Zr, Sn and Pb. A linear correlation between the Energy Weighted Sum Rule (EWSR) associated to PDR and the neutron skin thickness is evidenced. An increase of 15 MeV fm2 of EWSR to a change of 0.1 fm of neutron skin size is obtained. We conclude that different nuclei having close neutron skin size will exhaust the same EWSR in the pygmy region. Consequently a precise experimental estimate of total EWSR exhausted by PDR allows the determination of the neutron skin size and to constrain the slope parameter of the symmetry energy.
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url |
http://dx.doi.org/10.1051/epjconf/20146603004 |
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