Paper abstract bibtex

The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90% upper limit is ?_(GW) $\times$ [H_0/(72 km s\^ (?1) Mpc\^ (?1))]\^ 2 \ensuremath< 6.5 $\times$ 10\^ (-5). This is currently the most sensitive result in the frequency range 51-150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.

@article{caltechauthors43300, volume = {659}, number = {2}, month = {April}, author = {B. Abbott and R. Abbott and Rana X. Adhikari and J. Agresti and S. B. Anderson and M. Araya and H. Armandula and B. C. Barish and M. A. Barton and B. Bhawal and G. Billingsley and E. Black and K. Blackburn and R. Bork and D. A. Brown and D. Busby and L. Cardenas and C. Cepeda and P. Charlton and S. Chatterji and D. Coyne and T. D. Creighton and E. D'Ambrosio and R. DeSalvo and R. J. Dupuis and P. Ehrens and T. Etzel and M. Evans and L. Goggin and D. Grimmett and J. Heefner and P. Hoang and A. Ivanov and W. Kells and P. King and V. Kondrashov and D. Kozak and A. Lazzarini and M. Lei and K. Libbrecht and P. Lindquist and M. Mageswaran and K. Mailand and V. Mandic and E. Maros and J. N. Marx and S. Meshkov and D. Meyers and O. Miyakawa and M. Pedraza and P. Russell and M. Samidi and V. Sannibale and B. Sears and P. Shawhan and M. R. Smith and P. J. Sutton and M. Tarallo and R. Taylor and C. Torrie and W. Tyler and M. Varvella and S. Vass and A. Villar and S. J. Waldman and L. Wallace and R. Ward and D. Webber and A. J. Weinstein and S. E. Whitcomb and P. A. Willems and H. Yamamoto and L. Zhang and J. Zweizig and C. Cutler and Y. Pan and M. Vallisneri and K. S. Thorne and R. W. P. Drever}, note = {{\copyright} 2007 American Astronomical Society. Received 2006 September 21; accepted 2006 November 30. 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 Niedersachsen/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 National Aeronautics and Space Administration, the John Simon Guggenheim Foundation, the Alexander von Humboldt Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. LIGO DCC number: P060012-07-D.}, title = {Searching for a Stochastic Background of Gravitational Waves with the Laser Interferometer Gravitational-Wave Observatory}, publisher = {American Astronomical Society}, year = {2007}, journal = {Astrophysical Journal}, pages = {918--930}, keywords = {gravitational waves}, url = {http://resolver.caltech.edu/CaltechAUTHORS:20140110-072316825}, abstract = {The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90\% upper limit is ?\_(GW) {$\times$} [H\_0/(72 km s{\^{ }}(?1) Mpc{\^{ }}(?1))]{\^{ }}2 {\ensuremath{<}} 6.5 {$\times$} 10{\^{ }}(-5). This is currently the most sensitive result in the frequency range 51-150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.} }

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