Non-thermal synchrotron radiation in a strong magnetic field

Details Non-thermal synchrotron radiation in a strong magnetic field Non-thermal synchrotron radiation in a strong magnetic field

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..611b&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 611-614 (1984).

Physics

1

Radiation Mechanisms, Polarization, X-Ray Sources, X-Ray Bursts, Neutron Stars

Scientific paper

The synchrotron radiation spectra of mildly relativistic elecrons injected into strong fields (B~1012G) are calculated by a Monte Carlo technique. The energy losses, extremely rapid for such field strengths, are taken into account self-consistently. For photon energies below 1 MeV, the results are well fit by the product of a power law and an exponential, and the exponent and characteristic energy are tabulated with field strength and injection energy.

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