Abstract
In these lectures, the properties of dense hadronic and quark matter and its relation to compact stars will be discussed. In a bottom-up approach we start with nuclear and hypernuclear physics at low density and extrapolate 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 massradius relation of compact stars and the existence of a new family of solutions will be outlined.
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Schaffner-Bielich, J. (2004). Structure of Stars and Nuclei. In: Greiner, W., Itkis, M.G., Reinhardt, J., Güçlü, M.C. (eds) Structure and Dynamics of Elementary Matter. NATO Science Series, vol 166. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2705-5_23
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DOI: https://doi.org/10.1007/978-1-4020-2705-5_23
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