Isospin splitting of nucleon effective mass from giant resonances in Pb
arXiv:1507.04675 · doi:10.1103/PhysRevC.93.034335
Abstract
Based on mean field calculations with Skyrme interactions, we extract a constraint on the isovector effective mass in nuclear matter at saturation density , i.e., by combining the experimental data of the centroid energy of the isovector giant dipole resonance (IVGDR) and the electric dipole polarizability in Pb. Meanwhile, the isoscalar effective mass at is determined to be by analyzing the measured excitation energy of the isoscalar giant quadrupole resonance (ISGQR) in Pb. From the constrained and , we obtain the isospin splitting of nucleon effective mass in asymmetric nuclear matter of isospin asymmetry at as with the linear isospin splitting coefficient . We notice that using the recently corrected data on the in Pb with the contribution of the quasideuteron effect subtracted slightly enhances the isovector effective mass to and reduces the linear isospin splitting coefficient to . Furthermore, the constraints on , and at other densities are obtained from the similar analyses and we find that the increases with the density.
7 pages, 3 figures. New results and discussions added. Accepted version to appear in PRC
References in corpus (20)
- The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
- The neutron skin thickness from the measured electric dipole polarizability in Ni, Sn, and Pb
- Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- A new Skyrme interaction with improved spin-isospin properties
- Giant Quadrupole Resonances in 208Pb, the nuclear symmetry energy and the neutron skin thickness
- Isospin-dependent properties of asymmetric nuclear matter in relativistic mean-field models
- Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission
- Particle-vibration coupling effect on the -decay of magic nuclei
- Neutron-proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon-nucleus scattering data within an isospin dependent optical model
- Isovector properties of the Gogny interaction
- Thermal properties of asymmetric nuclear matter with an improved isospin- and momentum-dependent interaction
- Gamow-Teller response and its spreading mechanism in doubly magic nuclei
- Nuclear response theory with multiphonon coupling in a covariant framework
- Revisit of the neutron/proton ratio puzzle in intermediate-energy heavy-ion collisions
- Neutron-proton effective mass splitting in neutron-rich matter and its impacts on nuclear reactions
- Neutron-proton mass difference in finite nuclei and the Nolen-Schiffer anomaly
- Neutron-proton mass difference in isospin asymmetric nuclear matter
- Neutron-proton mass difference in nuclear matter
- Isospin splitting of nucleon effective mass and shear viscosity of nuclear matter
Cited by in corpus (32)
- Nuclear Equation of State from ground and collective excited state properties of nuclei
- Nucleon Effective Masses in Neutron-Rich Matter
- Dense Nuclear Matter Equation of State from Heavy-Ion Collisions
- Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
- Interdependence of different symmetry energy elements
- Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
- Constraining simultaneously nuclear symmetry energy and neutron-proton effective mass splitting with nucleus giant resonances from a dynamical approach
- Extended Skyrme interactions for nuclear matter, finite nuclei and neutron stars
- Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in Sn, Pb, and Ca
- Constraining the density dependence of the symmetry energy using the multiplicity and average ratios of charged pions
- Nucleonic metamodelling in light of multimessenger, PREX-II and CREX data
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
- Nuclear dipole polarizability from mean-field modeling constrained by chiral effective field theory
- Effect of isovector scalar meson on equation of state of dense matter within relativistic mean field model
- Constraining isovector nuclear interactions with giant resonances within a Bayesian approach
- Nuclear matter fourth-order symmetry energy in non-relativistic mean-field models
- Nucleus giant resonances from an improved isospin-dependent Boltzmann-Uehling-Uhlenbeck transport approach
- Bayesian uncertainty quantification for nuclear matter incompressibility
- Constraining isovector nuclear interactions with giant dipole resonance and neutron skin in Pb from a Bayesian approach
- Neutron-proton effective mass splitting in neutron-rich matter
- Entrainment effects in neutron-proton mixtures within the nuclear-energy density functional theory. I. Low-temperature limit
- Constraining nuclear matter parameters from correlation systematics:a mean-field perspective
- Bayesian inference of finite-nuclei observables based on the KIDS model
- The nucleon effective mass and its isovector splitting
- Bayesian inference on the isospin splitting of nucleon effective mass from giant resonances in Pb
- Correlations among symmetry energy elements in Skyrme models
- Isospin dependence of nucleon effective masses in neutron-rich matter
- Nuclear giant quadruple resonance within transport approach and its constraint on nucleon effective mass
- Revisiting the isospin relaxation time in intermediate-energy heavy-ion collisions
- In-medium potential, pion production in heavy-ion collisions and the symmetry energy
- Constraining neutron-proton effective mass splitting through nuclear giant dipole resonance within transport approach
- Phase-space excluded-volume approach for light clusters in nuclear medium