Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
arXiv:2007.01726 · doi:10.1088/1361-6471/aba423
Abstract
Properties of nuclear matter are investigated in the framework of relativistic Brueckner-Hartree-Fock model with the latest high-precision charge-dependent Bonn (pvCD-Bonn) potentials, where the coupling between pion and nucleon is adopted as pseudovector form. These realistic pvCD-Bonn potentials are renormalized to effective nucleon-nucleon () interactions, matrices. They are obtained by solving the Blankenbecler-Sugar (BbS) equation in nuclear medium. Then, the saturation properties of symmetric nuclear matter are calculated with pvCD-Bonn A, B, C potentials. The energies per nucleon are around MeV to MeV at saturation densities, fm to fm with these three potentials, respectively. It clearly demonstrates that the pseudovector coupling between pion and nucleon can generate reasonable saturation properties comparing with pseudoscalar coupling. Furthermore, these saturation properties have strong correlations with the tensor components of potentials, i.e., the -state probabilities of deuteron, to form a relativistic Coester band. In addition, the charge symmetry breaking (CSB) and charge independence breaking (CIB) effects are also discussed in nuclear matter from the partial wave contributions with these high-precision charge-dependent potentials. In general, the magnitudes of CSB from the differences between and potentials are about MeV, while those of CIB are around MeV from the differences between and potentials. Finally, the equations of state of asymmetric nuclear matter are also calculated with different asymmetry parameters. It is found that the effective neutron mass is larger than the proton one in neutron-rich matter.
arXiv comment32 pages, 11 figures, 5 tables, accepted by J. Phys. G
References in corpus (56)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- An accurate nucleon-nucleon potential with charge-independence breaking
- The equation of state for nucleon matter and neutron star structure
- The high-precision, charge-dependent Bonn nucleon-nucleon potential (CD-Bonn)
- Accurate Charge-Dependent Nucleon-Nucleon Potential at Fourth Order of Chiral Perturbation Theory
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- Construction of high-quality Nucleon-Nucleon potential models
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Equations of state for supernovae and compact stars
- Relativistic Equation of State of Nuclear Matter for Supernova and Neutron Star
- Quantum Monte Carlo methods for nuclear physics
- The two-nucleon system at next-to-next-to-next-to-leading order
- Coupled-cluster computations of atomic nuclei
- Self-consistent Green's function method for nuclei and nuclear matter
- The maximum mass and radius of neutron stars and the nuclear symmetry energy
- Relativistic Equation of State of Nuclear Matter for Supernova Explosion
- Precision nucleon-nucleon potential at fifth order in the chiral expansion
- High-quality two-nucleon potentials up to fifth order of the chiral expansion
- Semilocal momentum-space regularized chiral two-nucleon potentials up to fifth order
- The Nuclear Symmetry Energy
- Symmetry Energy I: Semi-Infinite Matter
- The Compression-Mode Giant Resonances and Nuclear Incompressibility
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Nuclear Equation of State from ground and collective excited state properties of nuclei
- Density-Dependent Relativistic Hartree-Fock Approach
- Relativistic Equation of State for Core-Collapse Supernova Simulations
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Shell Structure and -Tensor Correlations in Density-Dependent Relativistic Hartree-Fock theory
- Coupled-cluster calculations of nucleonic matter
- Peripheral nucleon-nucleon scattering at fifth order of chiral perturbation theory
- Self-consistent Green's functions formalism with three-body interactions
- Towards an ab initio covariant density functional for nuclear structure
- Microscopic calculations and energy expansions for neutron-rich matter
- Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT
- Delta isobars and nuclear saturation
- Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
- Bayesian modeling of the nuclear equation of state for neutron star tidal deformabilities and GW170817
- Complete relativistic equation of state for neutron stars
- The Microscopic Approach to Nuclear Matter and Neutron Star Matter
- Functional renormalization group studies of nuclear and neutron matter
- Equation of State of Nuclear Matter at high baryon density
- From asymmetric nuclear matter to neutron stars: a functional renormalization group study
- Fully self-consistent relativistic Brueckner-Hartree-Fock theory for finite nuclei
- Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817
- Nuclear matter properties from local chiral interactions with isobar intermediate states
- Nuclear matter properties with nucleon-nucleon forces up to fifth order in the chiral expansion
- Relativistic Brueckner-Hartree-Fock in nuclear matter without the average momentum approximation
- Relativistic Effects in Nuclear Matter and Nuclei
- Scalar and vector decomposition of the nucleon self-energy in the relativistic Brueckner approach
- Off-Shell Behavior of Nucleon Self-Energy in Asymmetric Nuclear Matter
- Nuclear and neutron matter equations of state from high-quality potentials up to fifth order of the chiral expansion
- Bayesian truncation errors in equations of state of nuclear matter with chiral nucleon-nucleon potentials
- The impact of charge symmetry and charge independence breaking on the properties of neutrons and protons in isospin-asymmetric nuclear matter
- The properties of neutron star from realistic nucleon-nucleon interaction within relativistic Hartree-Fock model
Cited by in corpus (4)
- Nuclear matter in relativistic Brueckner-Hartree-Fock theory with Bonn potential in the full Dirac space
- Neutron-proton effective mass splitting in neutron-rich matter
- Hadron-quark phase transition in neutron star by combining the relativistic Brueckner-Hartree-Fock theory and Dyson-Schwinger equation approach
- The nuclear symmetry energy from relativistic Brueckner-Hartree-Fock model