Symmetry energy properties of neutron-rich nuclei from the coherent density fluctuation model applied to nuclear matter calculations with Bonn potentials

We derive the values of nuclear symmetry energy, its components, as well as pressure in finite nuclei at saturation density from their corresponding values in nuclear matter obtained in nonrelativistic Brueckner-Hartree-Fock calculations with the realistic Bonn B and Bonn CD potentials using the coh...

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Detalles Bibliográficos
Autores: Danchev, I. C., Antonov, A. N., Kadrev, D. N., Gaidarov, M. K., Sarriguren, P., Moya de Guerra, Elvira
Tipo de recurso: artículo
Fecha de publicación:2020
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/6391
Acceso en línea:https://hdl.handle.net/20.500.14352/6391
Access Level:acceso abierto
Palabra clave:539.1
Strongly interacting particles
Many-body problem
Statistical-theory
Spin-isospin
State
Dependence
Equation
2-body
Parametrization
Saturation
Física nuclear
2207 Física Atómica y Nuclear
Descripción
Sumario:We derive the values of nuclear symmetry energy, its components, as well as pressure in finite nuclei at saturation density from their corresponding values in nuclear matter obtained in nonrelativistic Brueckner-Hartree-Fock calculations with the realistic Bonn B and Bonn CD potentials using the coherent density fluctuation model in the framework of a self-consistent Skyrme-Hartree-Fock plus BCS method. We focus on three isotopic chains of spherical nuclei (Ni, Sn, and Pb) and compare our results with those obtained with an effective Brueckner density-dependent potential. The role of the three-body forces on the considered quantities is also studied and discussed.