Signature of chaos in gravitational waves from a spinning particle
Shingo Suzuki, Kei-ichi Maeda

TL;DR
This paper investigates whether chaos in a spinning particle orbiting a black hole leaves detectable signatures in gravitational waves, revealing potential markers of chaos and system parameters.
Contribution
It demonstrates that chaotic orbits produce distinctive features in gravitational wave energy spectra, aiding in identifying chaos and system parameters.
Findings
Chaotic orbits emit about 10 times more gravitational energy than circular orbits.
Energy spectra of gravitational waves show characteristic features for chaotic orbits.
Enhanced energy emission is not always maximized in chaotic motion.
Abstract
A spinning test particle around a Schwarzschild black hole shows a chaotic behavior, if its spin is larger than a critical value. We discuss whether or not some peculiar signature of chaos appears in the gravitational waves emitted from such a system. Calculating the emitted gravitational waves by use of the quadrupole formula, we find that the energy emission rate of gravitational waves for a chaotic orbit is about 10 times larger than that for a circular orbit, but the same enhancement is also obtained by a regular "elliptic" orbit. A chaotic motion is not always enhance the energy emission rate maximally. As for the energy spectra of the gravitational waves, we find some characteristic feature for a chaotic orbit. It may tell us how to find out a chaotic behavior of the system. Such a peculiar behavior, if it will be found, may also provide us some additional informations to…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
