Graviton-photon scattering

N. E. J. Bjerrum-Bohr, Barry R. Holstein, Ludovic Planté, and Pierre Vanhove
Phys. Rev. D 91, 064008 – Published 3 March 2015

Abstract

We use the feature that the gravitational Compton scattering amplitude factorizes in terms of Abelian QED amplitudes to evaluate various gravitational Compton processes. We examine both the QED and gravitational Compton scattering from a massive spin-1 system by the use of helicity amplitude methods. In the case of gravitational Compton scattering we show how the massless limit can be used to evaluate the cross section for graviton-photon scattering and discuss the difference between photon interactions and the zero mass spin-1 limit. We show that the forward scattering cross section for graviton photoproduction has a very peculiar behavior, differing from the standard Thomson and Rutherford cross sections for a Coulomb-like potential.

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  • Received 30 October 2014

DOI:https://doi.org/10.1103/PhysRevD.91.064008

© 2015 American Physical Society

Authors & Affiliations

N. E. J. Bjerrum-Bohr1, Barry R. Holstein2, Ludovic Planté3, and Pierre Vanhove4

  • 1Niels Bohr International Academy and Discovery Center, The Niels Bohr Institute, Blegamsvej 17, DK-2100 Copenhagen Ø, Denmark
  • 2Department of Physics-LGRT, University of Massachusetts, Amherst, Massachusetts 01003, USA
  • 3Institut de Physique Théorique CEA, IPhT, F-91191 Gif-sur-Yvette, France and CNRS, URA 2306, F-91191 Gif-sur-Yvette, France
  • 4Institut des Hautes Études Scientifiques, F-91440 Bures-sur-Yvette, France

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Issue

Vol. 91, Iss. 6 — 15 March 2015

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