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Love Numbers for Rotating Black Holes in Higher Dimensions

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arxiv 2304.03743 v2 pith:XGP5QFSH submitted 2023-04-07 hep-th gr-qc

Love Numbers for Rotating Black Holes in Higher Dimensions

classification hep-th gr-qc
keywords blackholescoefficientsdimensionshigherlimitinglovenumbers
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We compute the tidal Love numbers and static response coefficients associated to several rotating black holes in higher dimensions, including Myers-Perry black holes, black rings, and black strings. These coefficients exhibit a rich and complex structure as a function of the black hole parameters and multipoles. Our results agree in limiting cases with known and new expressions for various lower-dimensional black holes. In particular, we provide an alternative approach to the computation of the static response of Kerr black holes as a limiting case of the boosted black string.

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Forward citations

Cited by 7 Pith papers

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

  1. Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms

    gr-qc 2026-06 unverdicted novelty 8.0

    Complete leading-order dynamical tidal corrections to neutron-star binaries are derived in EFT, showing dynamical Love numbers enhanced relative to static ones and yielding measurable contributions to the GW phase at ...

  2. Dynamical tidal Love numbers of black holes under generic perturbations: Connecting black hole perturbation theory with effective field theory

    gr-qc 2026-05 unverdicted novelty 7.0

    Dynamical tidal Love numbers for Kerr black holes are obtained to linear frequency order by matching EFT worldline couplings to black-hole perturbation solutions, including spin-induced mode mixing.

  3. 5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime

    hep-th 2025-05 unverdicted novelty 7.0

    Derives closed 5D partial-wave Raman scattering amplitude via NS functions and computes non-vanishing dynamical ℓ=0 and static ℓ=1 scalar tidal Love numbers with RG running up to O(G²) for STBH.

  4. Fermionic Love number of higher-dimensional Reissner-Nordstr\"om black holes

    gr-qc 2026-06 unverdicted novelty 6.0

    Fermionic tidal Love numbers for D-dimensional RN black holes remain nonzero for all angular momentum l (except extremal cases) and lose their l-dependence as D grows to infinity.

  5. Fermionic Love number of Reissner-Nordstr\"om black holes

    gr-qc 2025-10 unverdicted novelty 6.0

    Static fermionic tidal Love numbers are non-vanishing for non-extremal Reissner-Nordström black holes.

  6. Tidal deformation of an accreting compact object

    gr-qc 2026-07 conditional novelty 5.0

    For perfectly reflecting Schwarzschild-like ECOs, the log-compactness scaling of static scalar and spin-1 Love numbers survives a thin accretion disk, which mainly amplifies the response magnitude.

  7. Can wormholes have vanishing Love numbers?

    gr-qc 2026-05 unverdicted novelty 5.0

    For a specific R=0 wormhole, the magnetic Love number for ℓ=2 vanishes to linear order in the regularization parameter under static axial gravitational perturbations.