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

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Δημοσιευμένα: Ιαν 1, 2020
DOI: https://doi.org/10.12681/hnps.2638
T. Gaitanos
AUTh
G. Ferini
Catania
M. Colonna
INFN
M. Di Toro
INFN
G. A. Lalazissis
AUTh
H. H. Wolter
Περίληψη

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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Αναφορές
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