Generation mechanism of ultrahigh-energy gamma radiation in radio pulsars

Details Generation mechanism of ultrahigh-energy gamma radiation in radio pulsars Generation mechanism of ultrahigh-energy gamma radiation in radio pulsars

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55..761b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, USSR, Nov. 1-3, 1990) Akademiia Nauk SSSR, Izvestiia, Seriia Fizich

Computer Science

Gamma Rays, Particle Energy, Photons, Pulsars, Radiation Spectra, Crab Nebula, Neutron Stars, Spectral Methods, Stellar Magnetic Fields, Stellar Radiation, Stellar Rotation

Scientific paper

The spectrum of particles accelerated near the light cylinder of an axisymmetrically rotating magnetized neutron star is determined theoretically. Based on this spectrum, gamma radiation spectra are calculated for photon energies greater than 10 to the 11th eV. The theoretical spectra are compared with observations of the Crab and Vela pulsars.

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