Gravitational Raman Scattering: a Systematic Toolkit for Tidal Effects in General Relativity
Mikhail M. Ivanov, Yue-Zhou Li, Julio Parra-Martinez, Zihan Zhou

TL;DR
This paper develops a systematic framework using scattering amplitudes and effective field theory to compute tidal effects and Love numbers of compact objects in general relativity, clarifying previous ambiguities and extending to higher dimensions.
Contribution
It introduces a coordinate- and gauge-invariant method for calculating tidal Love numbers and dynamical effects using on-shell scattering amplitudes, including recoil effects and higher-dimensional extensions.
Findings
Leading static Love numbers vanish for black holes.
Dynamical Love numbers are non-zero and logarithmically run.
Love numbers in higher dimensions exhibit renormalization group running.
Abstract
We present a framework for systematic computations of scattering amplitudes for gravitational Raman scattering, -- the inelastic scattering of massless fields off compact relativistic objects. We focus on the small-frequency (post-Minkowskian, PM) regime relevant for the study of tidal effects, which can be mapped onto gravitational wave observables during the inspiraling phase of a merger. We demonstrate that this setup is ideal for systematic studies of tidal effects, in a way that is free from coordinate, gauge, and field redefinition ambiguities. We use a combination of worldline effective field theory, the background field method, and advanced scattering amplitude techniques to derive phase shifts for scattering of spin- fields off generic compact objects at third PM order. We demonstrate that the inclusion of the recoil of the object is crucial for consistency of this…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations · Cosmology and Gravitation Theories
