Constraints on the symmetry energy and neutron skins from experiments and theory

Understand

The symmetry energy contribution to the nuclear Equation of State (EoS) impacts various phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions.

• Its determination is a key objective of contemporary nuclear physics with consequences for the understanding of dense matter within neutron stars.
• We examine the results of laboratory experiments that have provided initial constraints on the nuclear symmetry energy and its density dependence at and somewhat below normal nuclear matter density.
• Some of these constraints have been derived from properties of nuclei.