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The symmetry energy from heavy ion reactions
2010
Proceedings of XLVIII International Winter Meeting on Nuclear Physics in Memoriam of Ileana Iori — PoS(BORMIO2010)
unpublished
The equation of state of asymmetric nuclear matter is an essential ingredient in nuclear physics and astrophysics but, as of today, insufficiently constrained by experiment. The symmetry energy, i.e. the difference between the energy of neutron matter and of symmetric matter, and its dependence on density are important for the modelling of neutron stars and supernova explosions as well as for isospin phenomena in nuclear reactions and nuclear structure. Heavy-ion reactions are a unique tool for
doi:10.22323/1.103.0061
fatcat:bcmbccc2ajdp3irdcluuabt4pq