Proton deceleration in a neutron star atmosphere

Details Proton deceleration in a neutron star atmosphere Proton deceleration in a neutron star atmosphere

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aipc...77..315k&link_type=abstract

In: Gamma ray transients and related astrophysical phenomena; Proceedings of the Workshop, La Jolla, CA, August 5-8, 1981. (A83-

Physics

Gamma Ray Bursts, Neutron Stars, Particle Acceleration, Stellar Atmospheres, X Ray Sources, Coulomb Collisions, Deceleration, Fokker-Planck Equation, Gyrofrequency, Plasma-Particle Interactions, Proton Energy, Proton Masers, Proton Scattering, Pulsars, Stellar Magnetic Fields

Scientific paper

The energy loss rate of fast protons in a strongly magnetized electron
gas has been calculated using the Fokker-Planck equation to describe the
dominant effect of small-angle Coulomb scattering. Stopping lengths of
order 1 gm/sq cm are obtained for 30 MeV protons and the possibility of
maser action at the gyrofrequency is indicated.

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