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- W3105342261 endingPage "012008" @default.
- W3105342261 startingPage "012008" @default.
- W3105342261 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." @default.
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- W3105342261 date "2014-03-18" @default.
- W3105342261 modified "2023-10-18" @default.
- W3105342261 title "Pygmies, giants, and skins as laboratory constraints on the equation of state of neutron-rich matter" @default.
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- W3105342261 doi "https://doi.org/10.1088/1742-6596/492/1/012008" @default.
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