Vanishing of quadratic Love numbers of Schwarzschild black holes

A bstract The induced conservative tidal response of self-gravitating objects in general relativity is parametrized in terms of a set of coefficients, which are commonly referred to as Love numbers. For asymptotically-flat black holes in four spacetime dimensions, the Love numbers are famously zero in the static regime. In this work, we show that this result continues to hold upon inclusion of nonlinearities in the theory for Schwarzschild black holes. We first solve the quadratic Einstein equations in the static limit to all orders in the multipolar expansion, including both even and odd perturbations. We show that the second-order solutions take simple analytic expressions, generically expressible in the form of finite polynomials. We then define the quadratic Love numbers at the level of the point-particle effective field theory. By performing the matching with the full solution in general relativity, we show that quadratic Love number coefficients are zero to all orders in the derivative expansion, like the linear ones.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-02-26
DOI
https://doi.org/10.1007/jhep02(2025)174
Citations
15
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
28.05
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article

Vanishing of quadratic Love numbers of Schwarzschild black holes

Luca Santoni, Simon Iteanu, Massimiliano Maria Riva, Filippo Vernizzi et al.
15 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
28.05
article

Vanishing of quadratic Love numbers of Schwarzschild black holes

Luca Santoni, Simon Iteanu, Massimiliano Maria Riva, Filippo Vernizzi, Nikola Savić
article en
15 citations

Abstract

A bstract The induced conservative tidal response of self-gravitating objects in general relativity is parametrized in terms of a set of coefficients, which are commonly referred to as Love numbers. For asymptotically-flat black holes in four spacetime dimensions, the Love numbers are famously zero in the static regime. In this work, we show that this result continues to hold upon inclusion of nonlinearities in the theory for Schwarzschild black holes. We first solve the quadratic Einstein equations in the static limit to all orders in the multipolar expansion, including both even and odd perturbations. We show that the second-order solutions take simple analytic expressions, generically expressible in the form of finite polynomials. We then define the quadratic Love numbers at the level of the point-particle effective field theory. By performing the matching with the full solution in general relativity, we show that quadratic Love number coefficients are zero to all orders in the derivative expansion, like the linear ones.

Journal of High Energy PhysicsVol. 2025(2)
École Normale Supérieure de Lyon (FR), Centre National de la Recherche Scientifique (FR), Université Paris Cité (FR), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Deutsches Elektronen-Synchrotron DESY (DE), Laboratoire AstroParticule et Cosmologie (FR), CEA Paris-Saclay (FR), Institut de Physique Théorique (FR), Columbia University (US)
Openalex Percentile: Top 0%
Black Holes and Theoretical Physics
28.05
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