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Neutron Star Mergers: Probing the EoS of Hot, Dense Matter by Gravitational Waves
2019
Particles
Gravitational waves, electromagnetic radiation, and the emission of high energy particles probe the phase structure of the equation of state of dense matter produced at the crossroad of the closely related relativistic collisions of heavy ions and of binary neutron stars mergers. 3 + 1 dimensional special- and general relativistic hydrodynamic simulation studies reveal a unique window of opportunity to observe phase transitions in compressed baryon matter by laboratory based experiments and by
doi:10.3390/particles2010004
fatcat:mafxv5z7j5bjdf4zjsmzuo7wny