Rotating black holes experience dynamical tides

Fuente: arXiv
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Auteurs principaux: Bhatt, Rajendra Prasad, Chakraborty, Sumanta, Bose, Sukanta
Format: Preprint
Publié: 2024
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author Bhatt, Rajendra Prasad
Chakraborty, Sumanta
Bose, Sukanta
author_facet Bhatt, Rajendra Prasad
Chakraborty, Sumanta
Bose, Sukanta
contents We find the dynamical tidal response of a Kerr black hole (BH) and demonstrate its tidal Love numbers to be non-vanishing when present in a non-axisymmetric external tidal field. To leading order, they depend quadratically on the black hole spin and linearly on the mode frequency. This implies that Kerr BHs are deformable under certain external, time-dependent perturbations. Since non-vanishing tidal Love numbers have been used in compact binary coalescences observed by the LIGO-Virgo-KAGRA (LVK) Collaboration to infer their non-BH nature, our findings have important implications on such inferences from future gravitational wave observations.
format Preprint
id arxiv_https___arxiv_org_abs_2406_09543
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Rotating black holes experience dynamical tides
Bhatt, Rajendra Prasad
Chakraborty, Sumanta
Bose, Sukanta
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We find the dynamical tidal response of a Kerr black hole (BH) and demonstrate its tidal Love numbers to be non-vanishing when present in a non-axisymmetric external tidal field. To leading order, they depend quadratically on the black hole spin and linearly on the mode frequency. This implies that Kerr BHs are deformable under certain external, time-dependent perturbations. Since non-vanishing tidal Love numbers have been used in compact binary coalescences observed by the LIGO-Virgo-KAGRA (LVK) Collaboration to infer their non-BH nature, our findings have important implications on such inferences from future gravitational wave observations.
title Rotating black holes experience dynamical tides
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2406.09543