Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters
General Relativity and Quantum Cosmology
2009-06-29 v1
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.
Keywords
Cite
@article{arxiv.0906.4968,
title = {Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters},
author = {Ivana Bochicchio and Mariafelicia De Laurentis and Ettore Laserra},
journal= {arXiv preprint arXiv:0906.4968},
year = {2009}
}
Comments
4 pages,3 figures,submitted for a book on New Frontiers in Fuzzy Logic and Complex Systems, Springer (2009)