paper

The Golden Era of Neutron Stars: from Hadrons to Quarks

arXiv:1902.01274 · doi:10.7566/JPSCP.26.011001

Abstract

Neutron stars were first posited in the early thirties, and discovered as pulsars in late sixties; however, only recently are we beginning to understand the matter they contain. This talk describes the continuing development of a consistent picture of the liquid interiors of neutron stars, driven by four advances: observations of two heavy neutron stars with masses 2.0 solar masses; inferences of masses and radii simultaneously for an increasing number of neutron stars in low mass X-ray binaries, and future determinations via the NICER observatory; the observation of the binary neutron star merger, GW170817, through gravitational waves as well as across the electromagnetic spectrum; and an emerging understanding in QCD of how nuclear matter can turn into deconfined quark matter in the interior. We describe the modern quark-hadron crossover equation of state, QHC18, and the corresponding neutron stars, which agree well with current observations.

6 pages, 6 figures, Proceedings, 8th Intl. Conference on Quarks and Nuclear Physics 2018 (Tsukuba, Japan), Nov. 2018

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