Slow Motion of Charges Interacting Through the Maxwell Field
arXiv:math-ph/0001002 · doi:10.1007/s002200000219
Abstract
We study the Abraham model for charges interacting with the Maxwell field. On the scale of the charge diameter, , the charges are a distance $\eps^{-1}R_ϕ$ apart and have a velocity $\sqrt{\eps} c$ with $\eps$ a small dimensionless parameter. We follow the motion of the charges over times of the order $\eps^{-3/2}R_ϕ/c$ and prove that on this time scale their motion is well approximated by the Darwin Lagrangian. The mass is renormalized. The interaction is dominated by the instantaneous Coulomb forces, which are of the order $\eps^{2}$. The magnetic fields and first order retardation generate the Darwin correction of the order $\eps^{3}$. Radiation damping would be of the order $\eps^{7/2}$.
Cited by in corpus (7)
- The Vlasov-Poisson system with radiation damping
- Mass and Spin Renormalization in Lorentz Electrodynamics
- Simplified models of electromagnetic and gravitational radiation damping
- Effective dynamics for particles coupled to a quantized scalar field
- Post-Coulombian Dynamics at Order 1.5
- The Vlasov limit and its fluctuations for a system of particles which interact by means of a wave field
- Post-Newtonian dynamics at order 1.5 in the Vlasov-Maxwell system