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Title: Photon-neutrino interactions

Abstract

The cross sections for the processes {gamma}{nu} {yields} {gamma}{gamma} {yields} {nu}{anti {nu}} are calculated with the aid of an effective Lagrangian derived from the Standard model. These cross sections are shown to be much larger than the elastic cross section {sigma}({gamma}{nu} {yields} {gamma}{nu}) for photon energies {omega} {ge} 1 keV. Possible astrophysical implications are discussed.

Authors:
 [1];  [2]
  1. Texas Univ., Austin, TX (United States)
  2. Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy
Publication Date:
Research Org.:
Texas Univ., Austin, TX (United States)
Sponsoring Org.:
USDOE Office of Energy Research, Washington, DC (United States); National Science Foundation, Washington, DC (United States)
OSTI Identifier:
555478
Report Number(s):
DOE/ER/40757-093; UTEXAS-HEP-97-2; MSUHEP-70205
ON: DE98001396; CNN: Grant PHY-93-07980; TRN: 98:008931
DOE Contract Number:
FG03-93ER40757
Resource Type:
Technical Report
Resource Relation:
Other Information: PBD: [1997]
Country of Publication:
United States
Language:
English
Subject:
66 PHYSICS; PHOTON-NEUTRINO INTERACTIONS; CROSS SECTIONS; LAGRANGIAN FUNCTION; ELASTIC SCATTERING; INELASTIC SCATTERING

Citation Formats

Dicus, D.A., and Repko, W.W. Photon-neutrino interactions. United States: N. p., 1997. Web. doi:10.2172/555478.
Dicus, D.A., & Repko, W.W. Photon-neutrino interactions. United States. doi:10.2172/555478.
Dicus, D.A., and Repko, W.W. 1997. "Photon-neutrino interactions". United States. doi:10.2172/555478. https://www.osti.gov/servlets/purl/555478.
@article{osti_555478,
title = {Photon-neutrino interactions},
author = {Dicus, D.A. and Repko, W.W.},
abstractNote = {The cross sections for the processes {gamma}{nu} {yields} {gamma}{gamma} {yields} {nu}{anti {nu}} are calculated with the aid of an effective Lagrangian derived from the Standard model. These cross sections are shown to be much larger than the elastic cross section {sigma}({gamma}{nu} {yields} {gamma}{nu}) for photon energies {omega} {ge} 1 keV. Possible astrophysical implications are discussed.},
doi = {10.2172/555478},
journal = {},
number = ,
volume = ,
place = {United States},
year = 1997,
month =
}

Technical Report:

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