1305.3202 (J. Piekarewicz)

Pygmies, giants, and skins as laboratory constraints on the equation of
state of neutron-rich matter    [PDF]

J. Piekarewicz

Laboratory experiments sensitive to the density dependence of the symmetry energy may place stringent constraints on the equation of state of neutron-rich matter and, thus, on the structure, dynamics, and composition of neutron stars. Understanding the equation of state of neutron-rich matter is a central goal of nuclear physics that cuts across a variety of disciplines. In this contribution I focus on how laboratory experiments on neutron skins and on both Pygmy and Giant resonances can help us elucidate the structure of neutron stars.

View original: http://arxiv.org/abs/1305.3202