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Radiative Friction for Charges Interacting with the Radiation Field: Classical Many-Particle Systems
[chapter]
Analysis, Modeling and Simulation of Multiscale Problems
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We consider an ensemble of classical particles modelled by means of a continuity equation for a distribution function which is coupled back to the self-induced fields. For such infinite dimensional systems simpler effective equations are derived in the limit c → ∞. A main emphasis is on higher order approximations, in particular on the first post-Newtonian order where radiation starts to play a role.
doi:10.1007/3-540-35657-6_19
fatcat:kmsda5j2hzayhdeyljsogamz2u