Authors: M. De Laurentis, S. Capozziello
Date: 26 Jun 2009
Abstract: 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.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis