Gravitational waves from stellar encounters
arXiv:0806.4117 · doi:10.1016/j.astropartphys.2008.07.005
Abstract
The emission of gravitational waves from a system of massive objects interacting on elliptical, hyperbolic and parabolic orbits is studied in the quadrupole approximation. Analytical expressions are then derived for the gravitational wave luminosity, the total energy output and gravitational radiation amplitude. A crude estimate of the expected number of events towards peculiar targets (i.e. globular clusters) is also given. In particular, the rate of events per year is obtained for the dense stellar cluster at the Galactic Center.
14 pages, 3 figures
References in corpus (7)
- Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects
- "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole
- Gravitational self force on a particle in circular orbit around a Schwarzschild black hole
- Higher-order gravity and the cosmological background of gravitational waves
- Gravitational waves from hyperbolic encounters
- Gravitational-wave background from compact objects embedded in AGN accretion disks
- Adiabatic Expansion for Metric Perturbation and the condition to solve the Gauge Problem for Gravitational Radiation Reaction Problem
Cited by in corpus (11)
- Classical Gravitational Bremsstrahlung from a Worldline Quantum Field Theory
- Constraining the electric charges of some astronomical bodies in Reissner-Nordstrom spacetimes and generic r^-2-type power-law potentials from orbital motions
- Gravitational wave energy spectrum of hyperbolic encounters
- Quadrupolar gravitational radiation as a test-bed for f(R)-gravity
- Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
- Spinning compact binary dynamics and chameleon orbits
- Radiative Classical Gravitational Observables at from Scattering Amplitudes
- Mimicking Mergers: Mistaking Black Hole Captures as Mergers
- Review of Pulsar Timing Array for Gravitational Wave Research
- Gravitomagnetic corrections on gravitational waves
- The Discovery Potential of Space-Based Gravitational Wave Astronomy