Towards a model-independent constraint of the high-density dependence of the symmetry energy
arXiv:1305.5417 · doi:10.1103/PhysRevC.88.044912
Abstract
Neutron-proton elliptic flow difference and ratio have been shown to be promising observables in the attempt to constrain the density dependence of the symmetry energy above the saturation point from heavy-ion collision data. Their dependence on model parameters like microscopic nucleon-nucleon cross-sections, compressibility of nuclear matter, optical potential, and symmetry energy parametrization is thoroughly studied. By using a parametrization of the symmetry energy derived from the momentum dependent Gogny force in conjunction with the Tübingen QMD model and comparing with the experimental FOPI/LAND data for 197Au+197Au collisions at 400 MeV/nucleon, a moderately stiff, x=-1.35 +/- 1.25, symmetry energy is extracted, a result that agrees with that of a similar study that employed the UrQMD transport model and a momentum independent power-law parametrization of the symmetry energy. This contrasts with diverging results extracted from the FOPI ratio available in the literature.
18 pages, 3 figures, accepted for publication in Phys. Rev. C
References in corpus (5)
- Symmetry energy from elliptic flow in 197Au + 197Au
- Systematics of pion emission in heavy ion collisions in the 1A GeV regime
- The neutron/proton ratio of squeezed-out nucleons and the high density behavior of the nuclear symmetry energy
- Dilepton production in heavy-ion collisions with in-medium spectral functions of vector mesons
- Probing the symmetry energy and the degree of isospin equilibrium
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