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Resonant Compton scattering in models of gamma-ray burst sources

Conference · · AIP Conference Proceedings (American Institute of Physics); (United States)
OSTI ID:5289336
 [1]
  1. Dept. of Physics, Lawrence Livermore National Laboratory, California 94550 (United States)

We consider here the spectra produced from the resonant Compton scattering of blackbody and power-law photons by a beam of relativistic electrons/positrons. The beam is assumed to be directed radially outward along the magnetic axis of a highly magnetized neutron star. We assume a dipole magnetic field geometry, and include the effects of magnetic Compton scattering energy losses on the particles in the beam during transport. A range of surface intensities for a magnetic field of 2[times]10[sup 12] Gauss is studied for a power-law electron/positron source function of index [Gamma]. The calculated scattered photon spectra are similar to observed gamma-ray burst spectra with a spectral index [alpha] which breaks from [alpha][congruent]1 to [Alpha][congruent][Gamma].

DOE Contract Number:
W-7405-ENG-48
OSTI ID:
5289336
Report Number(s):
CONF-9110310--
Journal Information:
AIP Conference Proceedings (American Institute of Physics); (United States), Journal Name: AIP Conference Proceedings (American Institute of Physics); (United States) Vol. 265:1; ISSN 0094-243X; ISSN APCPCS
Country of Publication:
United States
Language:
English