Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory
Abstract
We investigate how the quasi-universal relations connecting tidal deformability with gravitational waveform characteristics and/or properties of individual neutron stars that were proposed in the literature within general relativity would be influenced in the massive Damour-Esposito-Farese-type scalar-tensor gravity. For this purpose, we systematically perform numerical relativity simulations of ~120 binary neutron star mergers with varying scalar coupling constants. Although only three neutron-star equations of state are adopted, a clear breach of universality can be observed in the data sets. In addition to presenting difficulties in constructing quasi-universal relations in alternative gravity theories, we also briefly compare the impacts of non-general-relativity physics on the waveform features and those due to the first order or cross-over quantum chromodynamical phase transition.
Cite
@article{arxiv.2410.00137,
title = {Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory},
author = {Alan Tsz-Lok Lam and Yong Gao and Hao-Jui Kuan and Masaru Shibata and Karim Van Aelst and Kenta Kiuchi},
journal= {arXiv preprint arXiv:2410.00137},
year = {2024}
}