Abstract
The weak gravity conjecture indicates that extremal black holes in the low-energy effective field theory should be able to decay. This criterion gives rise to nontrivial constraints on the coefficients of higher-order derivative corrections to gravity. In this paper, we investigate the tidal deformability of neutral black holes due to higher-order derivative corrections. As a proof of concept, we consider a correction of cubic order in the Riemann curvature tensor. The tidal Love numbers of neutral black holes receive leading-order corrections from higher-order derivative terms, since black holes in pure General Relativity have vanishing tidal Love number. We conclude that the interplay between the tidal deformability of black holes and the weak gravity conjecture provides useful information about the effective field theory. © 2023 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.
| Original language | English |
|---|---|
| Article number | 044066 |
| Journal | Physical Review D |
| Volume | 108 |
| Issue number | 4 |
| Online published | 28 Aug 2023 |
| DOIs | |
| Publication status | Published - Aug 2023 |
| Externally published | Yes |
Funding
We thank L. Aalsma, A. Kehagias, D. Lombardo, T. Noumi, R. Penco, A. Riotto, I. Rothstein, L. Santoni, C. Vafa and M. Wiesner for interesting comments and discussions. V. D. L. is supported by funds provided by the Center for Particle Cosmology at the University of Pennsylvania. The work of J. K. and S. W. is supported in part by the DOE (HEP) Award No. DE-SC0013528.
Publisher's Copyright Statement
- This full text is made available under CC-BY 4.0. https://creativecommons.org/licenses/by/4.0/
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