Article
Upper Limits on a Stochastic Gravitational-wave Background Using LIGO and Virgo Interferometers at 600-1000 Hz
Physical Review D - Particles, Fields, Gravitation and Cosmology
Document Type
Article
Publication Date
6-4-2012
Disciplines
Abstract
A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the first joint search for a stochastic background using data from the LIGO and Virgo interferometers. In a frequency band of 600-1000 Hz, we obtained a 95% upper limit on the amplitude of ΩGW(f) ≥Ω3(f/900Hz)3, of Ω3
DOI
https://doi.org/10.1103/PhysRevD.85.122001
First Department
Physics
Acknowledgements
Retrieved February 1, 2021 from https://arxiv.org/pdf/1112.5004.pdf
Citation Information
J. Abadie, B. P. Abbott, R. Abbott, T. D. Abbott, et al.. "Upper Limits on a Stochastic Gravitational-wave Background Using LIGO and Virgo Interferometers at 600-1000 Hz" Physical Review D - Particles, Fields, Gravitation and Cosmology Vol. 85 Iss. 12 (2012) Available at: http://works.bepress.com/tiffany_summerscales/153/