Tidal Love numbers from EFT of black hole perturbations with timelike scalar profile

Abstract We study static tidal Love numbers (TLNs) of a static and spherically symmetric black hole for odd-parity metric perturbations. We describe black hole perturbations using the effective field theory (EFT), formulated on an arbitrary background with a timelike scalar profile in the context of scalar-tensor theories. In particular, we obtain a static solution for the generalized Regge-Wheeler equation order by order in a modified-gravity parameter and extract the TLNs uniquely by analytic continuation of the multipole index ℓ to non-integer values. For a stealth Schwarzschild black hole, the TLNs are vanishing as in the case of Schwarzschild solution in general relativity. We also study the case of Hayward black hole as an example of non-stealth background, where we find that the TLNs are non-zero (or there is a logarithmic running). This result suggests that our EFT allows for non-vanishing TLNs and can in principle leave a detectable imprint on gravitational waves from inspiralling binary systems, which opens a new window for testing gravity in the strong-field regime.

Authors

Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-09-01
DOI
https://doi.org/10.1088/1475-7516/2024/09/001
Citations
19
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
6.30
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article

Tidal Love numbers from EFT of black hole perturbations with timelike scalar profile

Kazufumi Takahashi, Shinji Mukohyama, Vicharit Yingcharoenrat, Naritaka Oshita et al.
19 citations
Journal of Cosmology and Astroparticle Physics
Pulsars and Gravitational Waves Research
6.30
article

Tidal Love numbers from EFT of black hole perturbations with timelike scalar profile

Kazufumi Takahashi, Shinji Mukohyama, Vicharit Yingcharoenrat, Naritaka Oshita, Chams Gharib Ali Barura, Hajime Kobayashi
article en
19 citations

Abstract

Abstract We study static tidal Love numbers (TLNs) of a static and spherically symmetric black hole for odd-parity metric perturbations. We describe black hole perturbations using the effective field theory (EFT), formulated on an arbitrary background with a timelike scalar profile in the context of scalar-tensor theories. In particular, we obtain a static solution for the generalized Regge-Wheeler equation order by order in a modified-gravity parameter and extract the TLNs uniquely by analytic continuation of the multipole index ℓ to non-integer values. For a stealth Schwarzschild black hole, the TLNs are vanishing as in the case of Schwarzschild solution in general relativity. We also study the case of Hayward black hole as an example of non-stealth background, where we find that the TLNs are non-zero (or there is a logarithmic running). This result suggests that our EFT allows for non-vanishing TLNs and can in principle leave a detectable imprint on gravitational waves from inspiralling binary systems, which opens a new window for testing gravity in the strong-field regime.

Journal of Cosmology and Astroparticle PhysicsVol. 2024(09)
Openalex Percentile: Top 3%
Pulsars and Gravitational Waves Research
6.30
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