POST-NEWTONIAN EXPANSION OF GRAVITATIONAL-WAVES FROM A PARTICLE IN CIRCULAR ORBIT AROUND A SCHWARZSCHILD BLACK-HOLE

Based upon the formalism recently developed by one of us (MS), we analytically perform the post-Newtonian expansion of gravitational waves from a test particle in circular orbit of radius gamma0 around a Schwarzschild black hole of mass M. We calculate gravitational wave forms and luminosity up to upsilon8 order beyond Newtonian, where upsilon = (M/r0)1/2. In particular, we give the exact analytical values of the coefficients of ln upsilon terms at upsilon6 and upsilon8 orders in the luminosity and confirm the numerical values obtained previously by one of us (HT) and Nakamura. Our result is valid in the small mass limit of one body and gives an important guideline for the gravitational wave physics of coalescing compact binaries.