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Searching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectors

Chow, Jong; Chua, Sheon; Inta, Ra; McClelland, David; Miller, John; Nguyen, Thanh; Scott, Susan M; Shaddock, Daniel; Slagmolen, Bram; Stochino, Alberto; Mavalvala, Nergis; Melatos, Andrew; Mendell, G; Meshkov, S; Mitrofanov, V P; Pedraza, M; Mittleman, R; Mueller, Guido; Munch, Jesper; Ottaway, D J; Wade, Andrew; Owen, Benjamin; Penn, S; Rajalakshmi, G; Reed, C M; Souradeep, T; Reitze, D; Riles, K; Schwinberg, P; Sammut, L; Sathyaprakash, B; Savage, R; Vocca, H; Saulson, P; Schofield, R; Sengupta, Anand S; Staley, A; Strigin, S; Summerscales, T.Z.; Susmithan, S; Tanner, D B; Torrie, Calum; Unnikrishnan, C S; Van Den Brand, J.; Shoemaker, D; Vass, S; Veitch, Peter John; Vorvick, C; Vyachanin, S; Waldman, Sam J; Wallace, L; Weinstein, A; Aasi, J; Ward, Robert; Wen, L; Abbott, T; Whiting, B F; Abadie, J; Abbott, B; Acernese, F; Adams, C; Adams, T; Adhikari, Rana; Allen, B; Anderson, S B; Anderson, WG; Beker, M G; Araya, M; Barsotti, L; Bulten, H.J.; Bartos, I; Basti, A; Bertolini, A; Beyersdorf, P T; Bilenko, I A; Billingsley, G; Blackburn, James Kent; Blom, M; Brau, J E; Bork, R; Charlton, Philip; Bose, S; Genin, E; Braginsky, V; Christensen, N; Coward, D; Coyne, D; Dhurandhar, S; Dumas, J-C; Ehrens, P; Etzel, T; Factourovich, M; Sigg, D; Korth, W. Zach; Fairhurst, S; Finn, Lee; Fritschel, Peter; Frolov, V; Giaime, J; Greenhalgh, R. J. S.; Gustafson, R; Heefner, J; Heptonstall, A; Kells, W; Iyer, B R; Jones, D I; Kawabe, Keita; King, P; Kissel, Jeffrey S; Kozak, D; Landry, M; Lazzarini, A; MacInnis, M; Mageswaran, M; Mailand, K; Sintes, A; Meadors, G.D.; Mandic, V.; Maros, E; Martynov, D; Marx, Jay

Description

Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors typically involve cross-correlating data from pairs of detectors. The sensitivity of such cross-correlation analyses depends, among other things, on the separation between the two detectors: the smaller the separation, the better the sensitivity. Hence, a colocated detector pair is more sensitive to a gravitational-wave background than a noncolocated detector pair. However, colocated detectors are also...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
URI: http://hdl.handle.net/1885/103186
Source: Physical Review D-Particles, Fields, Gravitation and Cosmology
DOI: 10.1103/PhysRevD.91.022003

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