Time domain calculation of the electromagnetic self-force on eccentric geodesics in Schwarzschild spacetime

Understand

I calculate the self-force acting on a particle with electric charge q moving on a generic geodesic around a Schwarzschild black hole.

• Using methods similar to those developed for the scalar field case discussed in a previous paper, I investigate the relative sizes of the conservative (half-advanced plus half-retarded) and dissipative (half-advanced minus half-retarded) pieces of the self-force.
• I also display the regularization parameters used in the mode-sum regularization scheme.