Summary.
We study the dynamics of N charges interacting with the Maxwell field. If their initial velocities are small compared to the velocity of light, c , then in lowest order their motion is governed by the static Coulomb Lagrangian. We investigate higher-order corrections with an explicit control on the error terms. The Darwin correction, order |v/c| 2 , has been proved previously. In this contribution we obtain the dissipative corrections due to radiation damping, which are of order |v/c| 3 relative to the Coulomb dynamics. If all particles have the same charge-to-mass ratio, the dissipation would vanish at that order.
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Received February 7, 2001; accepted September 21, 2001 Online publication November 30, 2001
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Kunze, M., Spohn, H. Post-Coulombian Dynamics at Order c-3. J. Nonlinear Sci. 11, 321–396 (2001). https://doi.org/10.1007/s00332-001-0455-z
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DOI: https://doi.org/10.1007/s00332-001-0455-z