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Structure of Stars and Nuclei

J. Schaffner-Bielich
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Abstract

The properties of dense hadronic and quark matter and its relation to compact stars are discussed. In a bottom-up approach one starts with nuclear and hypernuclear physics at low density and extrapolates hadronic matter to large densities. The matching to the quark matter phase is performed in a top-down approach starting at asymptotically large densities. Implications for the mass-radius relation of compact stars and the existence of a new family of solutions will be outlined.

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J. Schaffner-Bielich. 2004-03-10. Structure of Stars and Nuclei. https://arxiv.org/abs/astro-ph/0402597

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