Newton-like equations for a radiating particle
Alejandro Cabo Montes de Oca, Nana Geraldine Cabo-Bizet

TL;DR
This paper introduces Newton-like equations for a radiating particle that align with the Abraham-Lorentz-Dirac equations, avoiding runaway solutions and pre-acceleration, supported by numerical analysis and generalized modifications.
Contribution
It presents a new form of Newton equations for radiating particles that satisfy ALD equations and addresses issues like runaway solutions through smoothness conditions and effective forces.
Findings
Newton-like equations match ALD equations for general motions.
Numerical solutions confirm the absence of runaway and pre-acceleration effects.
Modified ALD equations handle discontinuous forces and support instantaneous force vanishing.
Abstract
Second order Newton equations of motion for a radiating particle are presented. It is argued that the trajectories obeying them also satisfy the Abraham-Lorentz-Dirac (ALD) equations for general 3D motions in the non-relativistic and relativistic limits. The case of forces only depending of the proper time is here considered. For these properties to hold, it is sufficient that the external force to be infinitely smooth and that a series formed with its time derivatives converges. This series define in a special local way the effective forces entering the Newton equations. When the external force vanishes in an open vicinity of a given time, the effective one also becomes null. Thus, the proper solutions of the effective equations can not show runaway or pre-acceleration effects. The Newton equations are numerically solved for a pulsed force given by an analytic function along the proper…
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