Department
Physics and Astronomy
Journal Title
Physical Review D
Publication Date
2004
Volume No.
69
Issue No.
102001
First Page
1
Last Page
21
Publisher
American Institute of Physics
File Name
005_Christensen-Nelson_FirstUpperLimitsFromLigoOnGravitationalWaveBursts.pdf
Abstract
We report on a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory ~LIGO! detectors. Our search focuses on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz. We bound the rate for such detected bursts at less than 1.6 events per day at a 90% confidence level. This result is interpreted in terms of the detection efficiency for ad hoc waveforms ~Gaussians and sine Gaussians! as a function of their root-sum-square strain hrss ; typical sensitivities lie in the range hrss ;10219–10217 strain/AHz, depending on the waveform. We discuss improvements in the search method that will be applied to future science data from LIGO and other gravitational wave detectors.
Rights Management
Carleton College does not own the copyright to this work and the work is available through the Carleton College Library following the original publisher's policies regarding self-archiving. For more information on the copyright status of this work, refer to the current copyright holder.
RoMEO Color
Green
Preprint Archiving
Yes
Postprint Archiving
Yes
Publisher PDF Archiving
Yes
Paid OA Option
Yes
Contributing Organization
Carleton College
Type
Article
Format
application/pdf
Language
English
DOI
10.1103/PhysRevD.69.102001
Recommended Citation
LIGO Scientific Collaboration, , and Nelson Christensen., "First upper limits from LIGO on gravitational wave bursts". Physical Review D, vol. 69, no. 102001, 2004. Available at: https://doi.org/10.1103/PhysRevD.69.102001. . [Online]. Accessed via Faculty Work. Physics and Astronomy. Carleton Digital Commons. https://digitalcommons.carleton.edu/phys_faculty/10
The definitive version is available at https://doi.org/10.1103/PhysRevD.69.102001