The effect of the gravitational constant variation on the phase of gravitational waves

Fuente: arXiv
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Main Authors: An, Jiachen, Sun, Bing, Cao, Zhoujian
Format: Preprint
Published: 2025
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author An, Jiachen
Sun, Bing
Cao, Zhoujian
author_facet An, Jiachen
Sun, Bing
Cao, Zhoujian
contents We have previously investigated the effect of the gravitational constant variation on the gravitational wave propagation. Pure theoretical analysis indicates that the leading order effect of the gravitational constant variation corrects the amplitude of gravitational waves, and the second order effect corrects the phase of gravitational waves. As the matched filtering technique is used by gravitational wave data analysis, the phase is more important than the amplitude. In the current paper we use LIGO-VIRGO-KAGRA data to constrain the gravitational constant variation. Our findings indicate that we need to wait until the distance of the detected gravitational wave events and/or the signal-to-noise ratio increases by $2n$ orders compared to the current detection state, and then we can use phase correction to get constraint $|\frac{G'}{G}|<10^{-n}$/yr for gravitational wave events without electromagnetic counterparts. For gravitational wave events with electromagnetic counterparts which provide the information of source's luminosity distance, the phase correction can almost always be neglected to constrain $\frac{G'}{G}$.
format Preprint
id arxiv_https___arxiv_org_abs_2508_21746
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The effect of the gravitational constant variation on the phase of gravitational waves
An, Jiachen
Sun, Bing
Cao, Zhoujian
General Relativity and Quantum Cosmology
We have previously investigated the effect of the gravitational constant variation on the gravitational wave propagation. Pure theoretical analysis indicates that the leading order effect of the gravitational constant variation corrects the amplitude of gravitational waves, and the second order effect corrects the phase of gravitational waves. As the matched filtering technique is used by gravitational wave data analysis, the phase is more important than the amplitude. In the current paper we use LIGO-VIRGO-KAGRA data to constrain the gravitational constant variation. Our findings indicate that we need to wait until the distance of the detected gravitational wave events and/or the signal-to-noise ratio increases by $2n$ orders compared to the current detection state, and then we can use phase correction to get constraint $|\frac{G'}{G}|<10^{-n}$/yr for gravitational wave events without electromagnetic counterparts. For gravitational wave events with electromagnetic counterparts which provide the information of source's luminosity distance, the phase correction can almost always be neglected to constrain $\frac{G'}{G}$.
title The effect of the gravitational constant variation on the phase of gravitational waves
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2508.21746