Radiation by ultrarelativistic electrons entering a dense medium in a strong magnetic field

Details Radiation by ultrarelativistic electrons entering a dense medium in a strong magnetic field Radiation by ultrarelativistic electrons entering a dense medium in a strong magnetic field

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..402k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, May 1986, p. 402-409) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

1

Electron Radiation, Electron Scattering, Neutron Stars, Stellar Magnetic Fields, Synchrotron Radiation, Electron Energy, Energy Dissipation, Field Strength, Radiation Spectra

Scientific paper

The synchrotron radiation of electrons with zero pitch angle before entering the matter is studied. Pitch-angle distribution occurs due to multiple scattering. It is shown that in the magnetic fields that are characteristic of pulsars the mechanism considered makes a main contribution to the electron energy losses in a wide range of the initial energies of the particles and concentrations of the nuclei.

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