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Searching for Kerr in the 2PM amplitude
Catholic Univ Louvain, Ctr Cosmol Particle Phys & Phenomenol CP3, Chemin Cyclotron 2, B-1348 Louvain La Neuve, Belgium..
Nordita SU.
CALTECH, Walter Burke Inst Theoret Phys, 1200 East Calif Blvd, Pasadena, CA 91125 USA..
2022 (engelsk)Inngår i: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, nr 7, artikkel-id 072Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

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) 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 spinning-2PM scattering to any order in the spin vectors of both objects; we present results here and in the supplementary material file 2PMSpin8Aux.nb up to eighth order in the spin vectors. Interestingly, despite leftover coefficients in the Compton amplitude, imposing the aforementioned relation between spin structures uniquely fixes some higher-spin parts of the 2PM amplitude.

sted, utgiver, år, opplag, sider
Springer Nature , 2022. nr 7, artikkel-id 072
Emneord [en]
Black Holes, Effective Field Theories, Scattering Amplitudes, Classical Theories of Gravity
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-316132DOI: 10.1007/JHEP07(2022)072ISI: 000824650500002Scopus ID: 2-s2.0-85134211733OAI: oai:DiVA.org:kth-316132DiVA, id: diva2:1686740
Merknad

QC 20220811

Tilgjengelig fra: 2022-08-11 Laget: 2022-08-11 Sist oppdatert: 2023-09-25bibliografisk kontrollert

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