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|a dc
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|a Wipf, Christopher C.
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|a Massachusetts Institute of Technology. Department of Physics
|e contributor
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|a MIT Kavli Institute for Astrophysics and Space Research
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|a Mavalvala, Nergis
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|a Zucker, Michael E.
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|a Wipf, Christopher C.
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|a Weiss, Rainer
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|a Waldman, Samuel J.
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|a Stein, Leo Chaim
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|a Stein, Andrew J.
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|a Smith, Nicolas de Mateo
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|a Shoemaker, David H.
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|a Shapiro, B.
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|a Sarin, P.
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|a Mittleman, Richard K.
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|a Mason, Kenneth R.
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|a Markowitz, Jared John
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|a MacInnis, Myron E.
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|a Katsavounidis, Erotokritos
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|a Hughey, Brennan J.
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|a Harry, Gregory
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|a Grimaldi, F.
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|a Goda, K.
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|a Fritschel, Peter K.
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|a Foley, Stephany
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|a Evans, Matthew J.
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|a Duke, I.
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|a Donovan, Frederick J.
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|a Corbitt, Thomas R.
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|a Cao, Junwei
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|a Brunet, G.
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|a Bodiya, Timothy Paul
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|a Blackburn, Lindy L.
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|a Barsotti, Lisa
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|a Mavalvala, Nergis
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|a Weiss, Rainer
|e author
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|a Waldman, Samuel J.
|e author
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|a Stein, Leo Chaim
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|a Stein, Andrew J.
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|a Smith, Nicolas de Mateo
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|a Shapiro, B.
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|a Sarin, P.
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|a Markowitz, Jared John
|e author
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|a Katsavounidis, Erotokritos
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|a Hughey, Brennan J.
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|a Harry, Gregory
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|a Grimaldi, F.
|e author
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|a Goda, K.
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|a Foley, Stephany
|e author
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|a Duke, I.
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|a Cao, Junwei
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|a Brunet, G.
|e author
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|a Blackburn, Lindy L.
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|a Barsotti, Lisa
|e author
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|a Mavalvala, Nergis
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|a Zucker, Michael E
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|a Shoemaker, David H
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|a Mittleman, Richard K
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|a Mason, Kenneth R
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|a MacInnis, Myron E
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|a Fritschel, Peter K
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|a Evans, Matthew J
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|a Donovan, Frederick J
|e author
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|a Corbitt, Thomas R
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|a Bodiya, Timothy P.
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|a First LIGO search for gravitational wave bursts from cosmic (super)strings
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|b American Physical Society,
|c 2010-02-26T16:54:01Z.
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|z Get fulltext
|u http://hdl.handle.net/1721.1/51835
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|a We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LIGO data from the fourth science run (S4) which took place in February and March 2005. No gravitational waves were detected in 14.9 days of data from times when all three LIGO detectors were operating. We interpret the result in terms of a frequentist upper limit on the rate of gravitational wave bursts and use the limits on the rate to constrain the parameter space (string tension, reconnection probability, and loop sizes) of cosmic string models. Many grand unified theory-scale models (with string tension Gμ/c[superscript 2]≈10[superscript -6]) can be ruled out at 90% confidence for reconnection probabilities p≤10[superscript -3] if loop sizes are set by gravitational back reaction.
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|a Research Corporation
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|a Alfred P. Sloan Foundation
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|a David and Lucile Packard Foundation
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|a Leverhulme Trust
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|a Alexander von Humboldt Foundation
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|a John Simon Guggenheim Foundation
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|a National Aeronautics and Space Administration
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|a Spanish Ministerio de Educacion y Ciencia
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|a Department of Science and Technology of India
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|a Council of Scientific and Industrial Research of India
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|a Natural Sciences and Engineering Research Council of Canada
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|a Australian Research Council
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|a State of Niedersachsen/Germany
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|a Max-Planck-Society
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|a Particle Physics and Astronomy Research Council of the United Kingdom
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|a United States National Science Foundation
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|a en_US
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|a Article
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|t Physical Review D
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