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Soft-photon emission effects and radiative corrections for electromagnetic processes at very high energies

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157154· OSTI ID:6143560
The effects of higher-order electromagnetic processes involving particles at ultrahigh energies are considered. Processes such as ''double Compton scattering'' (Compton scattering with the emission of an additional photon) are relevant for, for example, interaction of a high-energy electron with the cosmic blackbody photon gas. For incident photon energies greater than about 10/sup 13/ eV in the electron rest frame, the cross section for the process is as large as that for (ordinary) Compton scattering when the minimum energy of the additional outgoing photon is of the order of 0.01 mc/sup 2/, even though the process is of higher order. However, for certain problems, such as the energy loss for electrons through Compton scattering, the effects are largely cancelled by a negative contribution of the same order (in ..cap alpha..) from radiative corrections to Compton scattering. Because of its fundamental importance, a general outline of the physics of soft-photon emission is given for nonrelativistic and relativistic particle processes. In particular, the relationship between the classical and quantum-mechanical Bron-approximation formulae (which are essentially the same) is discussed.
Research Organization:
Department of Physics, University of California, San Diego
OSTI ID:
6143560
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 230:3; ISSN ASJOA
Country of Publication:
United States
Language:
English