Quadratic Quasi-Normal Modes of a Schwarzschild Black Hole

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Bucciotti, Bruno, Juliano, Leonardo, Kuntz, Adrien, Trincherini, Enrico
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866916520290942976
author Bucciotti, Bruno
Juliano, Leonardo
Kuntz, Adrien
Trincherini, Enrico
author_facet Bucciotti, Bruno
Juliano, Leonardo
Kuntz, Adrien
Trincherini, Enrico
contents Quadratic quasi-normal modes, generated at second order in black hole perturbation theory, are a promising target for testing gravity in the nonlinear regime with next-generation gravitational wave detectors. While their frequencies have long been known, their amplitudes remain poorly studied. We introduce regular variables and compute amplitudes for Schwarzschild black holes with the Leaver algorithm. We find a nonlinear ratio $\mathcal{R}\simeq0.154e^{-0.068i}$ for the most excited $\ell=4$ mode, matching results from Numerical Relativity. We also predict new low-frequency $\ell=2$ quadratic modes.
format Preprint
id arxiv_https___arxiv_org_abs_2405_06012
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Quadratic Quasi-Normal Modes of a Schwarzschild Black Hole
Bucciotti, Bruno
Juliano, Leonardo
Kuntz, Adrien
Trincherini, Enrico
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Theory
Quadratic quasi-normal modes, generated at second order in black hole perturbation theory, are a promising target for testing gravity in the nonlinear regime with next-generation gravitational wave detectors. While their frequencies have long been known, their amplitudes remain poorly studied. We introduce regular variables and compute amplitudes for Schwarzschild black holes with the Leaver algorithm. We find a nonlinear ratio $\mathcal{R}\simeq0.154e^{-0.068i}$ for the most excited $\ell=4$ mode, matching results from Numerical Relativity. We also predict new low-frequency $\ell=2$ quadratic modes.
title Quadratic Quasi-Normal Modes of a Schwarzschild Black Hole
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
High Energy Physics - Theory
url https://arxiv.org/abs/2405.06012