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Phys. Rev. D 59, 013012 (1998) [6 pages]

High energy photon-neutrino interactions

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Ali Abbasabadi1, Alberto Devoto2, Duane A. Dicus3, and Wayne W. Repko4
1Department of Physical Sciences, Ferris State University, Big Rapids, Michigan 49307
2Dipartmento di Fisica, Universitá di Cagliari and I.N.F.N., Sezione di Cagliari, Cagliari, Italy
3Center for Particle Physics and Department of Physics, University of Texas, Austin, Texas 78712
4Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824

Received 17 July 1998; published 8 December 1998

A general decomposition of the amplitudes for the 2⃗2 processes γνγν and γγνν̅ is obtained using gauge invariance and Bose symmetry. The restrictions implied by this decomposition are investigated for the reaction γγνν̅ by computing the one-loop helicity amplitudes in the standard model. In the center of mass, where s=2ω, the cross section grows roughly as ω6 up to the threshold for W-boson production, s=2mW. Astrophysical implications of very high energy photon-neutrino interactions are discussed.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.59.013012
DOI:
10.1103/PhysRevD.59.013012
PACS:
13.15.+g, 14.60.Lm, 14.70.Bh, 95.30.Cq