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

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 a...

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Main Authors: Bochicchio, I., De Laurentis, M., Laserra, E.
Format: Conference Proceeding
Language:English
Subjects:
Equations
Fuzzy systems
gravitational waves
Gravity
Kinematics
numerical gravity
Orbital calculations
Orbits (stellar)
Production
Stellar motion
theory of orbits
Velocity measurement
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De Laurentis, M.
Laserra, E.
description 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.
doi_str_mv 10.1109/FSKD.2009.654
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source IEEE Electronic Library (IEL) Conference Proceedings
subjects Equations
Fuzzy systems
gravitational waves
Gravity
Kinematics
numerical gravity
Orbital calculations
Orbits (stellar)
Production
Stellar motion
theory of orbits
Velocity measurement
title Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters
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