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## Banach Center Publications

1997 | 41 | 2 | 95-135
Tytuł artykułu

### The laser interferometer gravitational wave observatory project LIGO

Autorzy
Treść / Zawartość
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The Laser Interferometer Gravitational Wave Observatory (LIGO) will search for direct evidence of gravitational waves emitted by astrophysical sources in accord with Einstein's General Theory of Relativity. State of the art laser interferometers located in Hanford, Washington and Livingston Parish, Louisiana will unambiguously measure the infinitesimal displacements of isolated test masses which convey the signature of these gravitational waves. The initial implementation of LIGO will consist of three interferometers operating in coincidence to remove spurious terrestrial sources of noise. Construction of the facilities has begun at both sites, while research continues to design and develop the technologies to be utilized in achieving the target sensitivity curve having a minimum sensitivity of ∾ $1 × 10^{-19} meters/√Hz$ at ∾ 150 Hz for the initial phase of LIGO. Advanced LIGO interferometers of the future, having strain sensitivities on the order of $10^{-24}/√Hz$ corresponding to optical phase sensitivities on the order of $10^{-11} radians/√Hz$ over an observing band from 10 Hz to 10 kHz, require a complete understanding of the noise sources limiting detection. These fundamental noise sources will be quantitatively highlighted along with the principles of operation of the initial LIGO detector system and the characteristics of the most promising sources.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Numer
Strony
95-135
Opis fizyczny
Daty
wydano
1997
Twórcy
autor
• California Institute of Technology, Physics, Mathematics and Astronomy Division, LIGO Project, Mail Code 51-33, Pasadena, CA 91125, U.S.A.
Bibliografia
• [1] A. Abramovici, W. Althouse, R. Drever, Y. Gursel, S. Kawamura, F. Raab, D. Shoemaker, L. Seivers, R. Spero, K. Thorne, R. Vogt, R. Weiss, S. Whitcomb, M. Zuker, Science, 256, 325, (1992).
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• [7] Clifford M. Will and Alan G. Wiseman, to appear in Phys. Rev. D
• [8] J. Giame, 'Studies of Laser interferometer Design and a Vibration isolation System for Interferometric Gravitational Wave Detectors', Ph. D. thesis, MIT, (1995).
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• [10] Martin W. Regehr, 'Signal Extraction and Control for an Interferemetric Gravitational Wave Detector', Ph. D thesis, Caltech, (1995).
• [11] J. Giame, P. Saha, D. Shoemaker, L. Sievers, Rev. Sci. Instrum. 67 (1), 208, (1996).
• [12] P. R. Saulson, Fundamentals of Interferometric Gravitational Wave Detectors, New Jersey: Wold Scientific, (1994).
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• [18] T. Lyons and M. Regehr, 'Shot Noise in a Recycled Unbalanced LIGO', LIGO Technical Report, (1994).
• [19] Michael E. Zucker and Stanley E. Whitcomb, 'Measurement of Optical Path Fluctuations due to Residual Gas in the LIGO 40 Meter Interferometer', Marcel Grossman Proceedings, (1996).
• [20] Scott A. Hughes and Kip S. Thorne, 'Seismic Gravity Gradient Noise in Interferometric Gravitational Wave Detectors', in preparation, (1996).
• [21] A. Burrows, J. Hayes and B. A. Fryxell, to appear in Astrophys. J.
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• [23] Dong Lai, private communication, (1996).
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• [26] Benjamin J. Owen, Phys. Rev. D 53 6749 (1996).
• [27] B. S. Sathyaprakash, private communication, (1996).
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• [32] B. Allen, to appear in Proceedings of the Les Houches School on Astrophysical Sources of Gravitational Radiation, ed. Jean-Alain Marck, Springer Verlag, (1996).
• [33] Jean-Micheal Innocent and Bruno Torresani, this volume.
• [34] David Nicholson, preprint, (1995).
Typ dokumentu
Bibliografia
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