Characterization of the Ligo Input Optics System

Rong, Haisheng; Delker, T.; Mueller, G.; Rakhmanov, M.; Reitze, D. H.; Tanner, David; Yoshida, S.; Kells, Bill; Mavalvala, N.; Ottaway, D. J.; Sigg, D.; Whitcomb, S. E.; Adhikari, R. X.; Fritschel, P.; Zucker, M. E.

doi:10.1142/9789812777386_0399

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Possible Design Options For Aigo1

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Cited by 4 publications

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“…The IMC has been thoroughly studied 8,9 and the current design includes a suspended IMC. 10 However an optical fibre mode-cleaner studied by research institutes in France 11,12 could be included in the AIGO design at a later stage if successful.…”

Section: Possible Design Options For Aigomentioning

confidence: 99%

The Aigo Project

Li¹,

Blair²,

Davidson³

et al. 2011

Int. J. Mod. Phys. D

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Section: Possible Design Options For Aigomentioning

confidence: 99%

The Aigo Project

Li¹,

Blair²,

Davidson³

et al. 2011

Int. J. Mod. Phys. D

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“…Figure 6 shows the proposed optical layout for AIGO, including an input mode cleaner (IMC), a power recycling cavity (PRC), two arm cavities, a signal recycling cavity (SRC) and an output mode cleaner (OMC). The IMC has been thoroughly studied [17,18] and the current design includes a suspended IMC [19]; however, an optical fibre mode cleaner is being studied by research institutes in France and could be included in the AIGO design [20,21].…”

Section: Optical Configurationmentioning

confidence: 99%

AIGO: a southern hemisphere detector for the worldwide array of ground-based interferometric gravitational wave detectors

Barriga¹,

Blair²,

Coward³

et al. 2010

Class. Quantum Grav.

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This paper describes the proposed AIGO detector for the worldwide array of interferometric gravitational wave detectors. The first part of the paper summarizes the benefits that AIGO provides to the worldwide array of detectors. The second part gives a technical description of the detector, which will follow closely the Advanced LIGO design. Possible technical variations in the design are discussed.

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