Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data
arXiv:1207.7176 · doi:10.1103/PhysRevD.87.042001
Abstract
This paper presents results of an all-sky searches for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative ranges of [-2 x 10^-9, 1.1 x 10^-10] Hz/s for the fifth LIGO science run (S5). The novelty of the search lies in the use of a non-coherent technique based on the Hough-transform to combine the information from coherent searches on timescales of about one day. Because these searches are very computationally intensive, they have been deployed on the Einstein@Home distributed computing project infrastructure. The search presented here is about a factor 3 more sensitive than the previous Einstein@Home search in early S5 LIGO data. The post-processing has left us with eight surviving candidates. We show that deeper follow-up studies rule each of them out. Hence, since no statistically significant gravitational wave signals have been detected, we report upper limits on the intrinsic gravitational wave amplitude h0. For example, in the 0.5 Hz-wide band at 152.5 Hz, we can exclude the presence of signals with h0 greater than 7.6 x 10^-25 with a 90% confidence level.
29 pages, 14 figures, 6 tables. Science summary page at http://www.ligo.org/science/Publication-FullS5EatH/index.php ; Public access area to figures and tables at https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=p1200026
References in corpus (8)
- LIGO: The Laser Interferometer Gravitational-Wave Observatory
- The Breaking Strain of Neutron Star Crust and Gravitational Waves
- Maximum elastic deformations of compact stars with exotic equations of state
- Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run
- The Einstein@Home search for periodic gravitational waves in LIGO S4 data
- Exploiting Large-Scale Correlations to Detect Continuous Gravitational Waves
- Parameter-space metric of semicoherent searches for continuous gravitational waves
- Parameter-space correlations of the optimal statistic for continuous gravitational-wave detection