Symmetry energy I: Semi-infinite matter

Energy for a nucleus is considered in the macroscopic limit, in terms of nucleon numbers. Further considered for a nuclear system is the Hohenberg–Kohn energy functional, in terms of proton and neutron densities. Finally, Skyrme–Hartree–Fock calculations are carried out for a half-infinite particle-...

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Published inNuclear physics. A Vol. 818; no. 1; pp. 36 - 96
Main Authors Danielewicz, Paweł, Lee, Jenny
Format Journal Article
LanguageEnglish
Published Elsevier B.V 15.02.2009
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Abstract Energy for a nucleus is considered in the macroscopic limit, in terms of nucleon numbers. Further considered for a nuclear system is the Hohenberg–Kohn energy functional, in terms of proton and neutron densities. Finally, Skyrme–Hartree–Fock calculations are carried out for a half-infinite particle-stable nuclear-matter. In each case, the attention is focused on the role of neutron–proton asymmetry and on the nuclear symmetry energy. We extend the considerations on the symmetry term from an energy formula to the respective term within the Hohenberg–Kohn functional. We show, in particular, that in the limit of an analytic functional, and subject to possible Coulomb corrections, it is possible to construct isoscalar and isovector densities out of the proton and neutron densities, that retain a universal relation to each other, approximately independent of asymmetry. In the so-called local approximation, the isovector density is inversely proportional to the symmetry energy in uniform matter, at the local isoscalar density. Generalized symmetry coefficient of a nuclear system is related, in the analytic limit of the functional, to an integral of the isovector density. We test the relations, inferred from the Hohenberg–Kohn functional, in the Skyrme–Hartree–Fock calculations of half-infinite matter. Within the calculations, we obtain surface symmetry coefficients and parameters characterizing the densities, for the majority of Skyrme parameterizations proposed in the literature. The volume-to-surface symmetry-coefficient ratio, and the displacement of nuclear isovector relative to isoscalar surfaces, both strongly increase as the slope of symmetry energy, in the vicinity of normal density, increases.
AbstractList Energy for a nucleus is considered in the macroscopic limit, in terms of nucleon numbers. Further considered for a nuclear system is the Hohenberg–Kohn energy functional, in terms of proton and neutron densities. Finally, Skyrme–Hartree–Fock calculations are carried out for a half-infinite particle-stable nuclear-matter. In each case, the attention is focused on the role of neutron–proton asymmetry and on the nuclear symmetry energy. We extend the considerations on the symmetry term from an energy formula to the respective term within the Hohenberg–Kohn functional. We show, in particular, that in the limit of an analytic functional, and subject to possible Coulomb corrections, it is possible to construct isoscalar and isovector densities out of the proton and neutron densities, that retain a universal relation to each other, approximately independent of asymmetry. In the so-called local approximation, the isovector density is inversely proportional to the symmetry energy in uniform matter, at the local isoscalar density. Generalized symmetry coefficient of a nuclear system is related, in the analytic limit of the functional, to an integral of the isovector density. We test the relations, inferred from the Hohenberg–Kohn functional, in the Skyrme–Hartree–Fock calculations of half-infinite matter. Within the calculations, we obtain surface symmetry coefficients and parameters characterizing the densities, for the majority of Skyrme parameterizations proposed in the literature. The volume-to-surface symmetry-coefficient ratio, and the displacement of nuclear isovector relative to isoscalar surfaces, both strongly increase as the slope of symmetry energy, in the vicinity of normal density, increases.
Author Danielewicz, Paweł
Lee, Jenny
Author_xml – sequence: 1
  givenname: Paweł
  surname: Danielewicz
  fullname: Danielewicz, Paweł
  email: danielewicz@nscl.msu.edu
  organization: National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
– sequence: 2
  givenname: Jenny
  surname: Lee
  fullname: Lee, Jenny
  email: lee@nscl.msu.edu
  organization: National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
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ISSN 0375-9474
IngestDate Tue Jul 01 03:35:01 EDT 2025
Thu Apr 24 22:59:07 EDT 2025
Fri Feb 23 02:28:37 EST 2024
IsPeerReviewed true
IsScholarly true
Issue 1
Keywords Symmetry energy
Hohenberg–Kohn functional
21.65.-f
Skyrme–Hartree–Fock model
Isovector density
21.60.Jz
Half-infinite matter
Surface symmetry coefficient
21.10.Dr
21.10.Gv
21.65.Cd
21.65.Ef
Nuclear matter
Nuclear surface
Language English
License https://www.elsevier.com/tdm/userlicense/1.0
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c315t-211892d4f2a74f52c9925c7cbb4be7ea515501c2895103ae13998015ef568dc93
PageCount 61
ParticipantIDs crossref_citationtrail_10_1016_j_nuclphysa_2008_11_007
crossref_primary_10_1016_j_nuclphysa_2008_11_007
elsevier_sciencedirect_doi_10_1016_j_nuclphysa_2008_11_007
ProviderPackageCode CITATION
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PublicationCentury 2000
PublicationDate 2009-02-15
PublicationDateYYYYMMDD 2009-02-15
PublicationDate_xml – month: 02
  year: 2009
  text: 2009-02-15
  day: 15
PublicationDecade 2000
PublicationTitle Nuclear physics. A
PublicationYear 2009
Publisher Elsevier B.V
Publisher_xml – name: Elsevier B.V
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Snippet Energy for a nucleus is considered in the macroscopic limit, in terms of nucleon numbers. Further considered for a nuclear system is the Hohenberg–Kohn energy...
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StartPage 36
SubjectTerms Half-infinite matter
Hohenberg–Kohn functional
Isovector density
Nuclear matter
Nuclear surface
Skyrme–Hartree–Fock model
Surface symmetry coefficient
Symmetry energy
Title Symmetry energy I: Semi-infinite matter
URI https://dx.doi.org/10.1016/j.nuclphysa.2008.11.007
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