Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2009-02-19
AIP Conf.Proc.1128:131-143,2009
Physics
Nuclear Physics
Nuclear Theory
Talk given at the 5th ANL/MSU/JINA/INT FRIB Workshop on Bulk Nuclear Properties, MSU, Nov. 19-22, 2008, to appear in the AIP C
Scientific paper
10.1063/1.3146208
Heavy-ion reactions especially those induced by radioactive beams provide useful information about the density dependence of the nuclear symmetry energy, thus the Equation of State of neutron-rich nuclear matter, relevant for many astrophysical studies. The latest developments in constraining the symmetry energy at both sub- and supra-saturation densities from analyses of the isopsin diffusion and the $\pi^-/\pi^+$ ratio in heavy-ion collisions using the IBUU04 transport model are discussed. Astrophysical ramifications of the partially constrained symmetry energy on properties of neutron star crusts, gravitational waves emitted by deformed pulsars and the w-mode oscillations of neutron stars are presented briefly.
Chen Lie-Wen
Ko Che Ming
Krastev Plamen G.
Li Bao-An
Wen De-hua
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