Love beyond Einstein: Metric reconstruction and Love number in quadratic gravity using WEFT
Arpan Bhattacharyya, Saptaswa Ghosh, Naman Kumar, Shailesh Kumar, Sounak Pal
TL;DR
This work generalizes the tidal Love-number analysis to four-dimensional quadratic-curvature gravity using worldline EFT (WEFT). By diagonalizing the higher-derivative sector into scalar $Φ$ and tensor $Σ$ modes and reconstructing the metric from tree-level one-point functions, the authors show that quadratic corrections induce nonzero but scale-invariant tidal responses, with no classical RG running. They derive Yukawa-deformed solutions for scalar perturbations and perform UV–IR matching to fix ultraviolet charges, linking Wilson coefficients to observable tidal coefficients. Overall, the study provides a robust EFT framework to test deviations from GR with gravitational waves and clarifies how higher-curvature terms imprint in black hole tidal responses, including distinct Yukawa scales and controlled PN behavior.
Abstract
We study tidal Love numbers of static black holes in four-dimensional quadratic theory of gravity, extending the result of GR. We use worldline effective field theory (WEFT) methods to compute metric perturbations from one-point functions, treating the higher-derivative terms perturbatively. We show that insertions of scalar fields on the worldline induce non-zero tidal tails, and the corresponding Love number displays no RG running. The same conclusion holds for the insertions of tensor fields. Furthermore, for scalar dipole perturbations, we derive a Yukawa-deformed Frobenius solution and match the asymptotic behavior to fix the UV charge, finding agreement with EFT predictions of Wilson coefficients. Our work demonstrates that quadratic higher-curvature corrections induce non-zero but scale-independent tidal responses, offering a robust EFT framework to test deviations from GR in gravitational wave observations.
