Published November 25, 2005
| Published
Journal Article
Open
Upper Limits on a Stochastic Background of Gravitational Waves
- Creators
- Abbott, B.
- Abbott, R.
-
Adhikari, Rana X.
- Agresti, J.
- Anderson, S. B.
- Araya, M.
- Armandula, H.
- Barish, B. C.
- Barton, M. A.
- Bhawal, B.
-
Billingsley, G.
- Black, E.
- Blackburn, K.
- Bork, R.
-
Brown, D. A.
- Buonanno, A.
- Busby, D.
- Cardenas, L.
- Charlton, P.
- Chatterji, S.
-
Coyne, D.
- Creighton, T. D.
- D'Ambrosio, E.
- DeSalvo, R.
- Drever, R. W. P.
- Dupuis, R. J.
- Ehrens, P.
- Etzel, T.
- Evans, M.
- Goggin, L.
- Grimmett, D.
- Heefner, J.
- Hoang, P.
- Ivanov, A.
- Jones, L.
- Kells, W.
- King, P.
-
Kozak, D.
- Lazzarini, A.
- Lei, M.
-
Libbrecht, K.
- Lindquist, P.
- Liu, S.
- Mageswaran, M.
- Mailand, K.
- Mandic, V.
- Maros, E.
- Meshkov, S.
- Miyakawa, O.
- Nash, T.
- Nocera, F.
- Pedraza, M.
- Romie, J.
- Russell, P.
- Sanders, G. H.
- Sannibale, V.
- Sears, B.
- Shawhan, P.
- Smith, M. R.
- Sutton, P. J.
- Taylor, R.
- Thorne, K. S.
- Torrie, C.
- Tyler, W.
-
Vallisneri, M.
- Vass, S.
- Wallace, L.
- Ward, R.
- Webber, D.
- Whitcomb, S. E.
- Willems, P. A.
- Wilson, A.
- Yamamoto, H.
-
Zhang, L.
-
Zweizig, J.
- Pan, Y.
-
Weinstein, Alan J.
-
Chen, Y.
- LIGO Scientific Collaboration
Chicago
Abstract
The Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of Ω_0<8.4×10^(-4) in the 69–156 Hz band is ~10^5 times lower than the previous result in this frequency range.
Additional Information
© 2005 The American Physical Society. Received 30 July 2005; published 22 November 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedrersachsen, Germany, for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.Attached Files
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Additional details
- Eprint ID
- 23535
- Resolver ID
- CaltechAUTHORS:20110503-140518412
- NSF
- Max-Planck-Society
- Australian Research Council
- Natural Sciences and Engineering Research Council of Canada (NSERC)
- Council of Scientific and Industrial Research (India)
- Department of Science and Technology (India)
- Ministerio de Educacion y Ciencia (MEC)
- John Simon Guggenheim Foundation
- Leverhulme Trust
- David and Lucile Packard Foundation
- Research Corporation
- Alfred P. Sloan Foundation
- State of Niedersachsen/Germany
- Created
-
2011-05-03Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- TAPIR, LIGO