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arXiv · 1305.3202

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

J. Piekarewicz
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Abstract

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.

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J. Piekarewicz. 2013-05-14. Pygmies, giants, and skins as laboratory constraints on the equation of state of neutron-rich matter. https://doi.org/10.1088/1742-6596/492/1/012008

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