We study the impact of finite-temperature effects in numerical-relativity simulations of binary neutron star mergers with microphysical equations of state and neutrino transport in which we vary the effective nucleon masses in a controlled way. We find that, as the specific heat is increased, the merger remnants become colder and more compact due to the reduced thermal pressure support. Using a full Bayesian analysis, we demonstrate that this effect will be measurable in the postmerger gravitational wave signal with next-generation observatories at signal-to-noise ratios of 15.
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Abstract -
Kashyap, Rahul ; Das, Abhishek ; Radice, David ; Padamata, Surendra ; Prakash, Aviral ; Logoteta, Domenico ; Perego, Albino ; Godzieba, Daniel A. ; Bernuzzi, Sebastiano ; Bombaci, Ignazio ; et al ( , Physical Review D)
