Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters

Details Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters

2009-06-26

arxiv.org/abs/0906.4968v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages,3 figures,submitted for a book on New Frontiers in Fuzzy Logic and Complex Systems, Springer (2009)

Scientific paper

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.

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