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Tidal Love Numbers from EFT of Black Hole Perturbations with Timelike Scalar Profile

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arxiv 2405.10813 v2 pith:AXD3LFME submitted 2024-05-17 gr-qc hep-th

classification gr-qchep-th
keywords blackholetlnsperturbationsstaticbackgroundcaselove
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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 $\ell$ 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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Multipolar static tidal response of Schwarzschild black holes in cubic gravity: a metric-action derivation of tidal running

    gr-qc 2026-08 conditional novelty 7.0 of 10

    In cubic Weyl gravity, the metric-field derivation reproduces the known canonical electric beta functions, proves the quadrupole is the unique non-running electric multipole via an L-6 source factor, and gives explici...

  2. On the logarithmic Love number of black holes beyond general relativity

    gr-qc 2025-12 conditional novelty 6.0 of 10

    Logarithmic black hole Love numbers are fixed directly by the Taylor coefficients of the perturbation equation, and perturbative deviations from Schwarzschild/Reissner-Nordström force non-zero running.

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