Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory

Fuente: arXiv
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Main Authors: Lam, Alan Tsz-Lok, Gao, Yong, Kuan, Hao-Jui, Shibata, Masaru, Van Aelst, Karim, Kiuchi, Kenta
Format: Preprint
Published: 2024
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author Lam, Alan Tsz-Lok
Gao, Yong
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
author_facet Lam, Alan Tsz-Lok
Gao, Yong
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2410_00137
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory
Lam, Alan Tsz-Lok
Gao, Yong
Kuan, Hao-Jui
Shibata, Masaru
Van Aelst, Karim
Kiuchi, Kenta
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Nuclear Theory
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.
title Accessing universal relations of binary neutron star waveforms in massive scalar-tensor theory
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Nuclear Theory
url https://arxiv.org/abs/2410.00137