Gravitational waves from extreme mass-ratio inspirals in Dynamical Chern-Simons gravity

TL;DR

This paper explores how dynamical Chern-Simons gravity influences gravitational wave signals from extreme mass-ratio inspirals, showing that it increases energy flux and reduces waveform cycles, which can help constrain the theory with space-based detectors.

Contribution

It provides the first detailed analysis of Chern-Simons gravity effects on EMRI gravitational wave emissions using perturbation theory and Green's function methods.

Findings

Chern-Simons coupling increases total energy flux during inspiral.

The effect reduces the number of gravitational-wave cycles detectable.

Potential to constrain Chern-Simons coupling with LISA data.

Abstract

Dynamical Chern-Simons gravity is an interesting extension of General Relativity, which finds its way in many different contexts, including string theory, cosmological settings and loop quantum gravity. In this theory, the gravitational field is coupled to a scalar field by a parity-violating term, which gives rise to characteristic signatures. Here we investigate how Chern-Simons gravity would affect the quasi-circular inspiralling of a small, stellar-mass object into a large non-rotating supermassive black hole, and the accompanying emission of gravitational and scalar waves. We find the relevant equations describing the perturbation induced by the small object, and we solve them through the use of Green's function techniques. Our results show that for a wide range of coupling parameters, the Chern-Simons coupling gives rise to an increase in total energy flux, which translates into a fewer number of gravitational-wave cycles over a certain bandwidth. For space-based gravitational-wave detectors such as LISA, this effect can be used to constrain the coupling parameter effectively.