The GEO 600 gravitational wave detector
By B. Willke, P. Aufmuth, C. Aulbert, Stanislav Babak, R. Balasubramanian, B. Barr, S. Berukoff, S. Bose, G. Cagnoli, M. M. Casey and 60 more. 2002
306 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics
View Paper: https://www.semanticscholar.org/paper/ab6f5d83a4de28b838166e1350cb59dd9dc1f72e
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In Astronomy and Astrophysics
- Adam Burrows
- Christian D. Ott
- K. Kotake
- E. Livne
- Hans-Thomas Janka
- Bernhard Müller
- E. O’Connor
- J. Murphy
In Atomic and Molecular Physics, and Optics
- Giovanni Amelino-Camelia
- Adam Burrows
- E. Livne
- Rolf Walder
- Fabio Marchesoni
- Christian D. Ott
- L. Ferrarese
- K. Kotake
Citations in the corpus
- Explosion mechanism, neutrino burst and gravitational wave in core-collapse supernovae (2005, background): “For the details of each laser interferometer, see [8] for TAMA 300 (Mitaka, Japan), [366] for LIGO (Hanford, the United States), [376] for VIRGO (Pisa, Italy), and [387]”
- Supermassive Black Holes in Galactic Nuclei: Past, Present and Future Research (2004, background): “…wave observatories is already at work; the American LIGO (Barish 2000; Abbott, B. 2004), the British-German GEO600 detector (Danzmann, K. 1995; Willke et al. 2002; Abbott et al. 2004), the French-Italian VIRGO detector (Acernese et al. 2002), the Japanese TAMA300 detector (Ando et al. 2002),…”
- Quantum-Spacetime Phenomenology (2008, result): “I should note that at some point, in spite of its lack of maturity, this proposal started to attract some pronounced interest in relation to reports by the GEO600 interferometer [550] of unexplained excess noise [373]: it had been claimed [286] that Hogan’s version of holographic noise could match e”
- Status of VIRGO (2004, methodology): “Other detectors, such as LIGO [2], TAMA [3] and GEO [4], are based upon the same principle.”
- Gravitational Waves from Axisymmetric, Rotating Stellar Core Collapse (2003, background): “Gravitational waves couple so weakly to matter that they propagate almost undistorted from their source in the ultradense collapsing and rebounding stellar core to detectors like LIGO (Gustafson et al. 1999), VIRGO (Punturo 2003), GEO600 (Willke et al. 2002), and TAMA (Ando et al. 2001) on Earth.”
- Approximate Universal Relations for Neutron Stars and Quark Stars (2016, unknown): “The current most stringent constraints on dCS gravity come from Solar System observations of framedragging with LAGEOS [289] and Gravity Probe B [290, 291] and from table top experiments [292].”