Published May 2009
| Version v1
Journal article
Neutron skin of 208Pb and density dependence of the symmetry energy
Creators
- 1. Physics Department, University of Idaho, Moscow, Idaho 83844 (United States)
Description
We explore neutron skin predictions for 208Pb in relation to the symmetry pressure in various microscopic models based on realistic nucleon-nucleon potentials and either the Dirac-Brueckner-Hartree-Fock approach or the conventional Brueckner-Hartree-Fock framework implemented with three-body forces. We also discuss the correlation between the neutron skin and the radius of a fixed-mass neutron star.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevC.79.057301;
- arXiv
- arXiv:0812.4868v2;
Publishing Information
- Journal Title
- Physical Review. C, Nuclear Physics
- Journal Volume
- 79
- Journal Issue
- 5
- Journal Page Range
- p. 057301-057301.4
- ISSN
- 0556-2813
- CODEN
- PRVCAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41035309
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- CORRELATIONS; DENSITY; FORECASTING; HARTREE-FOCK METHOD; LEAD 208; MASS; NEUTRON STARS; NEUTRONS; NUCLEON-NUCLEON POTENTIAL; RELATIVISTIC RANGE; SIMULATION; SKIN; SYMMETRY; THREE-BODY PROBLEM
- Descriptors DEC
- APPROXIMATIONS; BARYONS; BODY; CALCULATION METHODS; ELEMENTARY PARTICLES; ENERGY RANGE; EVEN-EVEN NUCLEI; FERMIONS; HADRONS; HEAVY NUCLEI; ISOTOPES; LEAD ISOTOPES; MANY-BODY PROBLEM; NUCLEI; NUCLEONS; ORGANS; PHYSICAL PROPERTIES; POTENTIALS; STABLE ISOTOPES; STARS
Optional Information
- Notes
- (c) 2009 The American Physical Society