Authors: Ivana Bochicchio, Mariafelicia De Laurentis, Ettore Laserra
Date: 26 Jun 2009
Abstract: In this paper we investigate the gravitational waves emission by stellar dynamical structures as complex systems in the quadrupole approximation considering bounded and unbounded orbits. Precisely, after deriving analytical expressions for the gravitational wave luminosity, the total energy output and gravitational radiation amplitude, we present a computational approach to evaluate the gravitational wave-forms from elliptical, circular, parabolic and hyperbolic orbits as a function of Keplerian parameters.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis