Gravitational waves production from stellar encounters around massive black holes
by De Laurentis, M. and Capozziello, S.
6 pages, 3 figures; Multifrequency Behaviour of High-Energy Cosmic Sources, Vulcano Workshop 2009
The emission of gravitational waves from a system of massive objects interacting on elliptical, hyperbolic and parabolic orbits is studied in the quadrupole approximation. Analytical expressions are then derived for the gravitational wave luminosity, the total energy output and gravitational radiation amplitude. A crude estimate of the expected number of events towards peculiar targets (i.e. globular clusters) is also given. In particular, the rate of events per year is obtained for the dense stellar cluster at the Galactic Center.