Modeling the Complete Gravitational Wave Spectrum of Neutron Star Mergers
Sebastiano BernuzziDiFeST, University of Parma and INFN Parma, I-43124 Parma, ItalyTim DietrichTheoretical Physics Institute, University of Jena, 07743 Jena, GermanyAlessandro NagarInstitut des Hautes Etudes Scientifiques, 91440 Bures-sur-Yvette, France
2015en
ABI
Abstract
In the context of neutron star mergers, we study the gravitational wave spectrum of the merger remnant using numerical relativity simulations. Postmerger spectra are characterized by a main peak frequency f2 related to the particular structure and dynamics of the remnant hot hypermassive neutron star. We show that f(2) is correlated with the tidal coupling constant κ(2)^T that characterizes the binary tidal interactions during the late-inspiral merger. The relation f(2)(κ(2)^T) depends very weakly on the binary total mass, mass ratio, equation of state, and thermal effects. This observation opens up the possibility of developing a model of the gravitational spectrum of every merger unifying the late-inspiral and postmerger descriptions.
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