Strong radiative reaction in the non-linear Compton process

Details Strong radiative reaction in the non-linear Compton process Strong radiative reaction in the non-linear Compton process

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....41..169s&link_type=abstract

Astronomy and Astrophysics, vol. 41, no. 2, June 1975, p. 169-174.

Astronomy and Astrophysics

Astrophysics

6

Charged Particles, Compton Effect, Crab Nebula, Electromagnetic Fields, Particle Motion, Phase Velocity, Astronomical Models, Cosmic Plasma, Electrodynamics, Equations Of Motion, Group Velocity, Pulsars

Scientific paper

The transient behavior of the equations of motion of a charged particle undergoing strong radiative reaction under the influence of an intense electromagnetic field of given phase velocity is examined numerically. Analytical solutions are obtained for the steady oscillatory state for arbitrary phase velocity and field amplitude, and the solutions are used to obtain an estimate of the attenuation length scale for a strong wave propagating through a plasma with strong radiative reaction. The results are used to estimate the charge density required for spatial attenuation of the 30-Hz field in the Crab nebula.

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