Three-body force effect on nucleon momentum distributions in asymmetric nuclear matter within the framework of the extended BHF approach
arXiv:1301.3218 · doi:10.1103/PhysRevC.87.014314
Abstract
We have investigated the three-body force (TBF) effect on the neutron and proton momentum distributions in asymmetric nuclear matter within the framework of the extended Brueckner-Hartree-Fock approach by adopting the two-body interaction plus a microscopic TBF. In asymmetric nuclear matter, it is shown that the neutron and proton momentum distributions become different from their common distribution in symmetric nuclear matter. The predicted depletion of the proton hole states increases while the neutron one decreases as a function of isospin-asymmetry. The TBF effect on the neutron and proton momentum distributions turns out to be negligibly weak at low densities around and below the normal nuclear density. The TBF effect is found to become sizable only at high densities well above the saturation density, and inclusion of the TBF leads to an overall enhancement of the depletion of the neutron and proton Fermi seas.
9 pages, 4 figures
References in corpus (38)
- An accurate nucleon-nucleon potential with charge-independence breaking
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Self-consistent Green's function method for nuclei and nuclear matter
- Probing Cold Dense Nuclear Matter
- Asymmetric Nuclear Matter from Extended Brueckner-Hartree-Fock Approach
- Measurement of 2- and 3-Nucleon Short Range Correlation Probabilities in Nuclei
- Evidence for the Strong Dominance of Proton-Neutron Correlations in Nuclei
- Tensor Forces and the Ground-State Structure of Nuclei
- Investigation of Proton-Proton Short-Range Correlations via the 12C(e,e'pp) Reaction
- Interplay of Three-Body Interactions in the EOS of Nuclear Matter
- On the nuclear symmetry energy and the neutron skin in neutron-rich nuclei
- n-p Short-Range Correlations from (p,2p + n) Measurements
- Recent observation of short range nucleon correlations in nuclei and their implications for the structure of nuclei and neutron stars
- Correlations in Hot Asymmetric Nuclear Matter
- Isospin splitting of the nucleon mean field
- Correlated Strength in Nuclear Spectral Function
- Shear viscosity in neutron star cores
- Alpha-decay half-lives and Q_alpha values of superheavy nuclei
- Saturation of nuclear matter and short-range correlations
- Correlation between alpha-decay Energies of Superheavy Nuclei Involving Effect of Symmetry Energy
- A Self-Consistent Solution to the Nuclear Many-Body Problem at Finite Temperature
- Depletion of the nuclear Fermi sea
- Nuclear symmetry energy and the role of the tensor force
- Cooling of Akmal-Pandharipande-Ravenhall neutron star models
- Hot neutron matter from a Self-Consistent Green's Functions approach
- Nuclear structure studies with the 7Li(e,e'p) reaction
- In medium T-matrix for nuclear matter with three-body forces - binding energy and single particle properties
- Correlations and spectral functions in asymmetric nuclear matter
- Momentum Distribution in Nuclear Matter and Finite Nuclei
- Measurement of the 3He(e,e'p)pn reaction at high missing energies and momenta
- Transport parameters in neutron stars from in-medium NN cross sections
- The Nucleon Spectral Function at Finite Temperature and the Onset of Superfluidity in Nuclear Matter
- Self-consistent solution of Galitskii-Feynman equations at finite temperature
- One-body Properties of Nuclear Matter with Off-shell Propagation
- Two-Nucleon Momentum Distributions Measured in 3He(e,e'pp)n
- Self-energy Effects in the Superfluidity of Neutron Matter
- Minimal models of cooling neutron stars with accreted envelopes
- Transport equations and linear response of superfluid Fermi mixtures in neutron stars
Cited by in corpus (28)
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Nucleon Effective Masses in Neutron-Rich Matter
- Density and isospin asymmetry dependence of high-momentum components
- Correlated density-dependent chiral forces for infinite matter calculations within the Green's function approach
- 3PF2 pairing in high-density neutron matter
- The isospin quartic term in the kinetic energy of neutron-rich nucleonic matter
- Imprints of high-momentum nucleons in nuclei on hard photons from heavy-ion collisions around the Fermi Energy
- The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
- Constraining nucleon high momentum in nuclei
- Cross-checking the symmetry energy at high densities
- Nucleon momentum distributions in asymmetric nuclear matter
- Probing proton transition momentum in neutron-rich matter
- Taming nucleon density distributions with deep neural network method
- Proton-skins in momentum space and neutron-skins in coordinate space in heavy nuclei
- Effects of the high-momentum tail of nucleon momentum distribution on the isospin-sensitive observables
- Isospin dependence of nucleon effective masses in neutron-rich matter
- Nucleon Effective E-Mass in Neutron-Rich Matter from the Migdal-Luttinger Jump
- Effects of the initialization of nucleon momentum in heavy-ion collisions at medium energies
- Breakdown of the tensor component in the Skyrme energy density functional
- A local-density-approximation description of high-momentum tails in isospin asymmetric nuclei
- Precise Measurement of Short-Range Correlations in Nuclei from Bremsstrahlung Gamma Ray Emission in Low-Energy Heavy-Ion Collisions
- Nucleon momentum gap in asymmetric nuclear matter
- r-mode instability of neutron stars in low-mass X-ray binaries: effects of Fermi surface depletion and superfluidity of dense matter
- Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
- Experimental Study of Bremsstrahlung Gamma Ray Emission and Short-Range Correlations in Sn+Sn Collisions at 25 MeV/u
- Origins and Impacts of High-Density Symmetry Energy
- Effects of short-range correlations at high densities on neutron stars with and without DM content: role of the repulsive self-interaction
- Proton spectral functions in finite nuclei based on the extended Brueckner-Hartree-Fock approach