Searching for Kerr in the 2PM amplitude
Rafael Aoude, Kays Haddad, Andreas Helset

TL;DR
This paper derives all-spin Compton amplitudes in the classical limit for QED, QCD, and gravity, enabling higher-order spin calculations in 2PM scattering and fixing some higher-spin contributions through spin structure relations.
Contribution
It introduces spurious-pole-free, all-spin Compton amplitudes in the classical limit and extends the calculation of spinning 2PM scattering to eighth order in spin vectors.
Findings
Derived all-spin Compton amplitudes for QED, QCD, and gravity.
Extended spinning 2PM scattering calculations to eighth order in spin vectors.
Fixed some higher-spin contributions by imposing relations between spin structures.
Abstract
The classical scattering of spinning objects is well described by the spinor-helicity formalism for heavy particles. Using these variables, we derive spurious-pole-free, all-spin opposite-helicity Compton amplitudes (factorizing on physical poles to the minimal, all-spin three-point amplitudes of ref. \cite{Arkani-Hamed:2017jhn}) in the classical limit for QED, QCD, and gravity. The cured amplitudes are subject to deformations by contact terms, the vast majority of whose contributions we can fix by imposing a relation between spin structures -- motivated by lower spin multipoles of black hole scattering -- at the second post-Minkowskian (2PM) order. For QED and gravity, this leaves a modest number of unfixed coefficients parametrizing contact-term deformations, while the QCD amplitude is uniquely determined. Our gravitational Compton amplitude allows us to push the state-of-the-art of…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Superconducting Materials and Applications · Quantum Chromodynamics and Particle Interactions
