Simulations with a tunable phase-transition parameter in neutron-star equations of state produce unique post-merger gravitational-wave peaks and link Δp to the prompt-collapse mass threshold, with Δp ≲ 0.04 implied for GW170817.
Tolos, Dense hadronic matter in neutron stars, Acta Physica Polonica B 55, 1 (2024)
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Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers
Simulations with a tunable phase-transition parameter in neutron-star equations of state produce unique post-merger gravitational-wave peaks and link Δp to the prompt-collapse mass threshold, with Δp ≲ 0.04 implied for GW170817.