Cross-checking the symmetry energy at high densities
arXiv:1504.02528 · doi:10.1103/PhysRevC.93.044610
Abstract
The nuclear symmetry energy determines the birth of neutron stars and the elementary nucleosynthesis in the universe. To constrain the nuclear symmetry energy, besides the studies in astrophysics, many terrestrial nuclear experiments are being carried out using a wide variety of advanced new facilities. In this paper, by cross-checking two unrelated experimental measurements using the newly updated transport model, we obtained a slightly soft symmetry energy at supra-saturation nuclear densities. While extrapolating to low nuclear densities, this result is compatible with the recent finding by comparing the available data on the electric dipole polarizability with the theoretical predictions. Our finding is expected to push the studies of nuclear physics and astrophysics forward.
8 pages, 11 figures, PRC, in production
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Cited by in corpus (21)
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
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- The interplay of short-range correlations and nuclear symmetry energy in hard photon productions from heavy-ion reactions at Fermi energies
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- Blind spots of probing the high-density symmetry energy in heavy-ion collisions
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