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Constraints on EOS from finite nuclei, heavy ion collisions and neutron stars

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Published: Jan 1, 2020
DOI: https://doi.org/10.12681/hnps.2638
Keywords:
Nuclear matter equation of state symmetry energy finite nuclei heavy ion collisions strangeness ratio neutron stars maximum mass constraint proton fraction Direct Urca process
T. Gaitanos
AUTh
G. Ferini
Catania
M. Colonna
INFN
M. Di Toro
INFN
G. A. Lalazissis
AUTh
H. H. Wolter
Abstract

We present several possibilities offered by nuclear structure, the dynamics of intermediate energy heavy ion collisions and neutron stars to investigate the nuclear matter equation of state (EoS) beyond the ground state. In particular the high density nuclear EoS of asymmetric matter, i.e. the symmetry energy, is discussed.

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References
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