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

2009/06/26 by Ivana Bochicchio, Mariafelicia De Laurentis, Bochicchio, Ivana +3
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Pulsars and Gravitational Waves Research #Stellar, planetary, and galactic studies #gr-qc

paper · pdf · doi:10.48550/arxiv.0906.4968

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

arxiv created 2009/06/26 · openalex publication_date 2009/06/26 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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.

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