Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600–1000 Hz

Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600–1000 Hz

A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the...

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Bibliographic Details
Main Authors: Barsotti, Lisa, Bodiya, Timothy Paul, Corbitt, Thomas R., Donovan, Frederick J., Dwyer, Sheila Elizabeth, Evans, Matthew J., Foley, Stephany, Fritschel, Peter K., Harry, Gregory, Katsavounidis, Erotokritos, Kissel, Jeffrey S., MacInnis, Myron E., Mandel, Ilya, Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Mittleman, Richard K., Oelker, Eric Glenn, Shapiro, B., Shoemaker, David H., Soto, Jose M., Stein, Andrew J., Stein, Leo Chaim, Vaulin, Ruslan, Waldman, Samuel J., Weiss, R., Wipf, Christopher C., Zucker, Michael E.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Physical Society 2012
Online Access:http://hdl.handle.net/1721.1/72406
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187

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