Isospin dependence of nucleon effective mass in Dirac Brueckner-Hartree-Fock approach
arXiv:nucl-th/0412030 · doi:10.1016/j.physletb.2004.11.004
Abstract
The isospin dependence of the nucleon effective mass is investigated in the framework of the Dirac Brueckner-Hartree-Fock (DBHF) approach. The definition of nucleon scalar and vector effective masses in the relativistic approach is clarified. Only the vector effective mass is the quantity related to the empirical value extracted from the analysis in the nonrelatiistic shell and optical potentials. In the relativistic mean field theory, where the nucleon scalar and vector potentials are both energy independent, the neutron vector potential is stronger than that of proton in the neutron rich nuclear matter, which produces a smaller neutron vector effective mass than that of proton. It is pointed out that the energy dependence of nucleon potentials has to be considered in the analysis of the isospin dependence of the nucleon effective mass. In the DBHF the neutron vector effective mass is larger than that of proton once the energy dependence of nucleon potentials is considered. The results are consistent with the analysis of phenomenological isospin dependent optical potentials.
4 pages, 3 Postscript figures
References in corpus (5)
- Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
- Transport properties of isospin effective mass splitting
- Correlations and the Dirac Structure of the Nucleon Self-Energy
- Relativistic Structure of the Nucleon Self-Energy in Asymmetric Nuclei
- Effective DBHF Method for Asymmetric Nuclear Matter and Finite Nuclei
Cited by in corpus (34)
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Nucleon-nucleon cross sections in neutron-rich matter and isospin transport in heavy-ion reactions at intermediate energies
- The Nuclear Symmetry Energy
- Neutron Stars and the Nuclear Equation of State
- The equation of state for dense nucleonic matter from a metamodeling. I. Foundational aspects
- Density-Dependent Relativistic Hartree-Fock Approach
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Nucleon Effective Masses in Neutron-Rich Matter
- Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals
- From Brueckner Approach to Skyrme-type Energy Density Functional
- Isospin-dependent properties of asymmetric nuclear matter in relativistic mean-field models
- Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
- Thermal properties of hot and dense matter with finite range interactions
- Thermal properties of asymmetric nuclear matter with an improved isospin- and momentum-dependent interaction
- Isospin splitting of nucleon effective mass from giant resonances in Pb
- Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
- Effects of isospin and momentum dependent interactions on thermal properties of asymmetric nuclear matter
- High-energy behavior of the nuclear symmetry potential in asymmetric nuclear matter
- Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions Induced by Neutron-Rich Nuclei
- Neutron-proton effective mass splitting and thermal evolution in neutron rich matter
- Nuclear symmetry potential in the relativistic impulse approximation
- Phase Transition of Finite Size Quark Droplets with Isospin Chemical Potential in the Nanbu--Jona-Lasinio Model
- Neutron-proton effective mass splitting in neutron-rich matter and its impacts on nuclear reactions
- Proton radioactivity with a Yukawa effective interaction
- Nonrelativistic nucleon effective masses in nuclear matter: BHF versus RHF
- Two-body contributions to the effective mass in nuclear effective interactions
- Isospin-asymmetric nuclear matter
- Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction
- A phenomenological equation of state for isospin asymmetric nuclear matter
- Bayesian inference on the isospin splitting of nucleon effective mass from giant resonances in Pb
- Comparison of different relativistic models applied to dense nuclear matter
- Prediction of the excitation energies of the 2 states for superheavy nuclei based on the microscopically derived Grodzins relation
- Relativistic Hartree-Fock Chiral Lagrangians with confinement, nucleon finite size and short-range effects
- Three-body Force Effects on the Properties of Neutron-rich Nuclear Matter