Relativistic electrons in pulsar magnetospheres - Quantum corrections to the classical regime

Details Relativistic electrons in pulsar magnetospheres - Quantum corrections to the classical regime Relativistic electrons in pulsar magnetospheres - Quantum corrections to the classical regime

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.251..681d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 251, Aug. 15, 1991, p. 681-686. Research supported by J

Mathematics

Logic

6

Pulsars, Relativistic Plasmas, Stellar Magnetospheres, Electron Energy, Quantum Electrodynamics, Radiative Transfer

Scientific paper

A classical description of the motion of plasmas in pulsar magnetospheres has been developed following the single-particle approach. It is shown that this description needs to take into account quantum corrections due to radiative effects. Instead of deterministic trajectories stochastic ones are found, and it is shown that radiative effects are stronger than expected.

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