A note on the gravitational wave energy spectrum of parabolic and hyperbolic encounters
arXiv:2001.05187 · doi:10.1088/1361-6382/ab6be2
Abstract
The first calculation of the frequency spectrum of gravitational wave mass quadrupole radiation for binaries on hyperbolic orbits was performed in arXiv:1207.5359. Some shortcomings of their derivation were pointed out, but there are still inaccuracies and supplements that we believe are worthwhile to communicate. In this note we provide a consistent and straightforward exposition of the frequency spectrum in the case of hyperbolic encounters and explicitly determine the parabolic limit, which was not possible with the previous treatments.
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Cited by in corpus (14)
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- The stochastic gravitational wave background from close hyperbolic encounters of primordial black holes in dense clusters
- Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
- Observables from classical black hole scattering in Scalar-Tensor theory of gravity from worldline quantum field theory
- Frequency space derivation of linear and non-linear memory gravitational wave signals from eccentric binary orbits
- Radiative Classical Gravitational Observables at from Scattering Amplitudes
- Effects of orbital precession on hyperbolic encounters
- Detectability of stochastic gravitational wave background from weakly hyperbolic encounters
- Gravitational bremsstrahlung in plasmas and clusters
- Mass octupole and current quadrupole corrections to gravitational wave emission from close hyperbolic encounters
- Gravitational wave background from primordial black holes in globular clusters
- Interactions among binary black holes in star clusters: Eccentric gravitational wave captures and triple formation
- Frequency domain analysis of the gravitational wave energy loss in hyperbolic encounters
- Energetics and scattering of gravitational two-body systems at fourth post-Minkowskian order