LIGO Document P1300154-v24

Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009-2010 LIGO and Virgo Data

Document #:
Document type:
P - Publications
Submitted by:
Eric Thrane Send email
Updated by:
S. Gwynne Crowder Send email
Document Created:
16 Sep 2013, 10:12
Contents Revised:
03 Jul 2014, 07:41
Metadata Revised:
03 Jul 2014, 07:41
Actually Revised:
11 Jul 2014, 07:06
Other Versions:
27 Jun 2014, 16:30
Gravitational-wave sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the universe that is unavailable through standard astrophysical observations, making its study of fundamental importance to understanding the evolution of the universe. The latest data from LIGO and Virgo display no evidence of a stochastic gravitational-wave signal so we place direct 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5-1726 Hz. In the frequency band of 41.5-169.25 Hz, we constrain the energy density of the stochastic background, Omega_GW(f), to be less than 5.6x10^-6. For the 600-1000 Hz band, Omega_GW(f) is less than 0.14(f/900 Hz)^3, a factor of 2.5 lower than the best previously reported upper limits. Moreover, we found Omega_GW(f) to be less than 1.8x10^-4 for 170-600 Hz and less than 1.0(f/1300 Hz)^-3 for 1000-1726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the detection of inflationary gravitational waves.
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