Abstract
This talk reviews current understanding of the states of matter in the liquid interior of neutron stars — including nuclear matter, pion and kaon condensation, and normal and strange quark matter — and their effect on neutron star structure and dynamics. Learning about high density matter in the laboratory by means of ultrarelativistic heavy-ion collisions is also discussed.
Supported in part by NSF Grant DMR88-18713.
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Baym, G. (1991). The High Density Interiors of Neutron Stars. In: Ventura, J., Pines, D. (eds) Neutron Stars: Theory and Observation. NATO ASI Series, vol 344. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3536-8_2
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