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Nuclear symmetry energy components and their ratio: A new approach within the coherent density fluctuation model

dc.contributor.authorGaidarov, M. K.
dc.contributor.authorMoya de Guerra, Elvira
dc.contributor.authorAntonov, A. N.
dc.contributor.authorDanchev, I. C.
dc.contributor.authorSarriguren, P.
dc.contributor.authorKadrev, D. N.
dc.date.accessioned2023-06-16T14:17:24Z
dc.date.available2023-06-16T14:17:24Z
dc.date.issued2021-10-11
dc.description©2021 American Physical Society. A.N.A, M.K.G., and D.N.K. are grateful for the support of the Bulgarian National Science Fund under Contract No. KP-06-N38/1. I.C.D also wishes to acknowledge partial financial support from the University of Mount Olive Professional Development Fund. P.S. acknowledges support from Ministerio de Ciencia e Innovacion MCIU/AEI/FEDER,UE (Spain) under Contract No. PGC2018-093636-B-I00.
dc.description.abstractA different alternative approach to calculate the ratio of the surface to volume components of the nuclear symmetry energy is proposed in the framework of the coherent density fluctuation model (CDFM). An alternate expression (scheme II) for the ratio is derived consistently within the model. This expression appears in a form more direct and physically motivated than the expression (scheme I) that was used in our previous works within the CDFM and avoids preliminary assumptions and mathematical ambiguities in scheme I. The calculations are based on the Skyrme and Brueckner energy-density functionals for nuclear matter and on the nonrelativistic Brueckner-Hartree-Fock method with realistic Bonn B and Bonn CD nucleon-nucleon potentials. The approach is applied to isotopic chains of Ni, Sn, and Pb nuclei using nuclear densities obtained in self-consistent Hartree-Fock+BCS calculations with the SLy4 Skyrme effective interaction. The applicability of both schemes within the CDFM is demonstrated by a comparison of the results with the available empirical data and with results of other theoretical studies of the considered quantities. Although in some instances the results obtained for the studied ratio and the symmetry energy components are rather close in both schemes, the proposed scheme II leads to more realistic values that agree better with the empirical data and exhibits conceptual and operational advantages.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia e Innovación (MICINN)/FEDER
dc.description.sponsorshipBulgarian National Science Fund
dc.description.sponsorshipUniversity of Mount Olive Professional Development Fund
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/68784
dc.identifier.doi10.1103/PhysRevC.104.044312
dc.identifier.issn2469-9985
dc.identifier.officialurlhttps://doi.org/10.1103/PhysRevC.104.044312
dc.identifier.relatedurlhttps://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/4539
dc.issue.number4
dc.journal.titlePhysical review C
dc.language.isoeng
dc.publisherAmer Physical Soc
dc.relation.projectIDPGC2018-093636-B-I00
dc.relation.projectIDKP-06-N38/1
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordStatistical-theory
dc.subject.keywordNatural orbitals
dc.subject.keywordDistributions
dc.subject.keywordMomentum
dc.subject.keywordMatter
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleNuclear symmetry energy components and their ratio: A new approach within the coherent density fluctuation model
dc.typejournal article
dc.volume.number104
dspace.entity.typePublication

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