Finding Fields and Self-Force in a Gauge Appropriate to Separable Wave Equations II

Gravitational waves from the inspiral of a stellar-sized black hole in to a supermassive black hole are an important source for the Laser Interferometer Space Antenna. A method for computing self force has been proposed that uses regularizes solutions of the Teukolsky equation [1]. The prescription is outlined in the previous talk. In this talk, I focus on computational details for a particle in circular orbit in a Schwarzschild spacetime. \newline [1] T.\ S.\ Keidl, J.\ L.Friedman, and A.\ G.\ Wiseman, Phys. Rev. D. {\bf 75}, 124009 (2007); gr-qc/0611072.