Authors: S. Capozziello, M. De Laurentis, F.De Paolis, G. Ingrosso, A. Nucita
Date: 30 Dec 2007
Abstract: The emission of gravitational waves from a system of massive objects interacting on hyperbolic orbits is studied in the quadrupole approximation. Analytic expressions are derived for the gravitational radiation luminosity, the total energy output and the gravitational radiation amplitude. An estimation of the expected number of events towards different targets (i.e. globular clusters and the center of the Galaxy) is also given. In particular, for a dense stellar cluster at the galactic center, a rate up to one event per year is obtained.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis