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On higher-derivative effects on the gravitational potential and particle bending

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arxiv 1905.05657 v4 pith:UJWDYAWF submitted 2019-05-14 hep-th gr-qc

classification hep-thgr-qc
keywords bendingclassicalamplitudeanglecasecomputedeformationgravitational
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Using modern amplitude techniques we compute the leading classical and quantum corrections to the classical gravitational potential between two massive scalars induced by adding an $R^3$ term to Einstein gravity. We then study the scattering of massless scalars, photons and gravitons off a heavy scalar in the presence of the same $R^3$ deformation, and determine the bending angle in the three cases from the non-analytic component of the scattering amplitude. Similarly to the Einstein-Hilbert case, we find that the classical contribution to the bending angle is universal, but unlike that case, universality is preserved also by the first quantum correction. Finally we extend our analysis to include a deformation of the form $\Phi R^2$, where $\Phi$ is the dilaton, which arises in the low-energy effective action of the bosonic string in addition to the $R^3$ term, and compute its effect on the graviton bending.

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Cited by 3 Pith papers

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  1. Dynamical Love Numbers for Black Holes and Beyond from Shell Effective Field Theory

    hep-th 2025-12 accept novelty 8.0 of 10

    A shell-based EFT computes scalar Love numbers for Schwarzschild black holes through O(G^9) and conjectures an all-orders Riemann-zeta structure.

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    hep-th 2026-08 conditional novelty 7.0 of 10

    In modified-gravity theories, spin Hall deflection of light and gravitational waves by a spinning black hole becomes non-commuting, so a ray disperses into a blob, and black-hole spin direction can tighten causality b...

  3. Running Love Numbers and the Effective Field Theory of Gravity

    hep-th 2025-01 conditional novelty 7.0 of 10

    Higher-derivative gravity corrections induce non-zero, classically running tidal Love numbers for black holes, computed here with a new tidal Green function method.

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