http://arxiv.org/abs/2305.08401
The investigation of the phase state of dense matter is hindered by complications of first-principle nonperturbative quantum chromodynamics. By performing the first consistent general-relativistic calculations of tidal-excited g-mode of neutron stars with a first-order strong interaction phase transition in the high-density core, we demonstrate that gravitational wave signal during binary neutron star inspiral probes their innermost hadron-quark transition and provides potent constraints from present and future gravitational-wave detectors.
Z. Miao, E. Zhou and A. Li
Tue, 16 May 23
51/83
Comments: 5 pages, 3 figures, 6 pages supplemental material