6533b7dcfe1ef96bd1272182
RESEARCH PRODUCT
Computational Approach to Gravitational Waves Forms in Stellar Systems as Complex Structures through Keplerian Parameters
Ivana BochicchioEttore LaserraMariafelicia De Laurentissubject
PhysicsPhysics::General PhysicsGravitational waveFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Gravitational accelerationGeneral Relativity and Quantum CosmologyGravitational energyGeneral Relativity and Quantum CosmologyClassical mechanicsStandard gravitational parameterGravitational fieldStellar dynamicsQuadrupoleAstrophysics::Earth and Planetary AstrophysicsGravitational redshiftdescription
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.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2009-06-26 |