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In this paper we investigate the gravitational waves emission by stellardynamical structures as complex systems in the quadrupole approximationconsidering bounded and unbounded orbits. Precisely, after deriving analyticalexpressions for the gravitational wave luminosity, the total energy output andgravitational radiation amplitude, we present a computational approach toevaluate the gravitational wave-forms from elliptical, circular, parabolic andhyperbolic orbits as a function of Keplerian parameters.

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