A gravitational wave observatory operating beyond the quantum shot-noise limit

A gravitational wave observatory operating beyond the quantum shot-noise limit

Around the globe several observatories are seeking the first direct detection of gravitational waves (GWs). These waves are predicted by Einstein's general theory of relativity and are generated, for example, by black-hole binary systems. Present GW detectors are Michelson-type kilometre-scale...

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Main Authors: Barsotti, Lisa (Author), Bodiya, Timothy P. (Author), Corbitt, Thomas R (Author), Donovan, Frederick J (Author), Dwyer, S. (Author), Evans, Marshall (Author), Foley, Stephany (Author), Fritschel, Peter K (Author), Harry, Gregory (Author), Katsavounidis, Erotokritos (Author), Kissel, Jeffrey S. (Author), MacInnis, Myron E (Author), Mandel, Ilya (Author), Mason, Kenneth R (Author), Matichard, Fabrice (Author), Mavalvala, Nergis (Author), Mittleman, Richard K (Author), Oelker, Eric Glenn (Author), Sankar, S. (Author), Shapiro, B. (Author), Shoemaker, David H (Author), Smith, N. D. (Author), Soto, J. (Author), Stein, Abraham (Author), Vaulin, Ruslan (Author), Waldman, Samuel J. (Author), Weiss, Rainer (Author), Wipf, Christopher C. (Author), Zucker, Michael E (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), Lincoln Laboratory (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Springer Nature America, Inc, 2019-06-03T16:35:40Z.
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