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Future Gravitational Wave Detectors
2020In this chapter, we discuss the future of gravitational wave detectors beyond the present second generation (2G). Several ambitious third generation (3G) projects which will significantly increase the reach of the detectors, through increased sensitivity as well as the ability to detect gravitational waves with lower frequencies, are being planned ...
Ajit Kembhavi, Pushpa Khare
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Skyhook gravitational-wave detector
Nature, 1985Gravitational waves in the 10â100-mHz band are inaccessible to Earth-based detectors because of seismic noise. Hitherto, the most sensitive detectors in this frequency band have been the Doppler tracking of interplanetary spacecraft1 and excitations of seismic motions in the Earth's surface2,3.
Vladimir B. Braginsky, Kip S. Thorne
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European gravitational wave detector falters
Science, 2017Fragile glass fibers hurt Virgo's chances to observe in 2017 with U.S. counterpart.
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SPACECRAFT GRAVITATIONAL WAVE DETECTORS
International Journal of Modern Physics D, 2011For detecting gravitational waves in space, deep-space laser ranging using drag-free spacecraft is a common method. Deep space provides a large arena and a long integration time. Laser technology provides measurement sensitivity, while drag-free technology ensures gravitational phenomenon to be measured with least spurious noises.
PENG DONG, WEI-TOU NI
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The Virgo Gravitational Wave Detector
Frontiers in Optics 2009/Laser Science XXV/Fall 2009 OSA Optics & Photonics Technical Digest, 2009The interferometer spectral-density of resolution is 6 x 10-231/ âHZ at 250 Hz.. We show the performances of mirror surfaces and coatings, laser frequency and amplitude stabilizations, interferometer control. We discuss advanced Virgo optical-technologies.
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Interferometric gravitational wave detectors
International Journal of Modern Physics D, 2018Gravitational wave detection has now entered the era in which signals are being found. It is timely, therefore, to review the current detectors and how they work. This review focuses on the dramatic arc that links the earliest clear understanding of gravitational wave detection with the current generation of detectors.
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Cryogenic gravitational wave detectors
Physica B: Condensed Matter, 2000Abstract Direct detection of gravitational waves is one of the great challenges of contemporary experimental physics. Gravitational waves provide unique information about the coherent bulk motion of the matter in the Universe and constitute a powerful testing ground for theories of gravity. After 40 years from the beginning of the experimental search
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New Class of Gravitational Wave Detectors
Nature, 1971IN a series of classic articles, Weber1â3 derived the equations of motion and the response of mass quadrupole detectors to tensor gravitational waves. He has also constructed a detector which is a cylindrical rod tuned to its fundamental longitudinal acoustic resonance. These devices (class 1 detectors) have a definite relationship between the resonant
D H, Douglass, J A, Tyson
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Spherical resonant-mass gravitational wave detectors
Physical Review D, 1995A spherical gravitational wave antenna is a very promising detector for gravitational wave astronomy because it has a large cross section, isotropic sky coverage, and can provide the capability of determining the wave direction. In this paper we discuss several aspects of spherical detectors, including the eigenfunctions and eigenfrequencies of the ...
, Zhou, , Michelson
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Interferometric gravitational wave detectors
Nuclear Physics B - Proceedings Supplements, 2005The status, progress and plans for the interferometer gravitational wave detectors are presented. Interferometric gravitational wave detectors are complementary to the resonant detectors. Interferometers are broadband detectors covering a frequencies range of about 10 to 10 4 Hz and are generally sensitive to lower frequency sources or different ...
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