Isospin Diffusion in Heavy-Ion Collisions and the Neutron Skin Thickness of Lead
arXiv:nucl-th/0505051 · doi:10.1103/PhysRevC.72.041601
Abstract
The correlation between the thickness of the neutron skin in Pb-208, and the degree of isospin diffusion in heavy-ion collisions is examined. The same equation of state is used to compute the degree of isospin diffusion in an isospin-depedent transport model and the neutron skin thickness in the Hartree-Fock approximation. We find that skin thicknesses less than 0.15 fm are excluded by the isospin diffusion data.
5 pages, 4 figures; few minor corrections and updates; version to appear in PRC
References in corpus (3)
Cited by in corpus (34)
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
- Neutron and Proton Transverse Emission Ratio Measurements and the Density Dependence of the Asymmetry Term of the Nuclear Equation of State
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy
- Neutron skin thickness in droplet model with surface width dependence: indications of softness of the nuclear symmetry energy
- Pygmy dipole resonance as a constraint on the neutron skin of heavy nuclei
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Pygmy Resonances and Neutron Skins
- Isospin-dependent properties of asymmetric nuclear matter in relativistic mean-field models
- Neutron density distributions from antiprotonic 208Pb and 209Bi atoms
- Locating the inner edge of neutron star crust using terrestrial nuclear laboratory data
- Origin of the neutron skin thickness of 208Pb in nuclear mean-field models
- Difference in proton radii of mirror nuclei as a possible surrogate for the neutron skin
- Expanding Nuclear Physics Horizons with the Gamma Factory
- Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in Sn, Pb, and Ca
- Thermal effects on nuclear symmetry energy with a momentum-dependent effective interaction
- Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
- Probing the Nuclear Symmetry Energy with Heavy-Ion Reactions Induced by Neutron-Rich Nuclei
- The neutron/proton ratio of squeezed-out nucleons and the high density behavior of the nuclear symmetry energy
- Constraining properties of rapidly rotating neutron stars using data from heavy-ion collisions
- Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data
- Isospin dependent properties of asymmetric nuclear matter
- Nuclear symmetry potential in the relativistic impulse approximation
- Neutron-proton bremsstrahlung from intermediate energy heavy-ion reactions as a probe of the nuclear symmetry energy?
- Isospin dependent thermodynamics of fragmentation
- Nuclear symmetry energy effects on neutron stars properties
- A phenomenological equation of state for isospin asymmetric nuclear matter
- Symmetry energy dependence of long timescale isospin transport
- Effects of neutron-skin thickness on direct hard photon emission from reactions induced by the neutron-rich projectile Ca
- From nuclear reactions to compact stars: a unified approach
- Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
- Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions
- Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories