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- W1666589112 abstract "All the long baseline interferometers for the detection of gravitational radiation which are presently being studied are based on the construction of a large, Michelson-like interferometer with an armlength of 1 to 4 km, containing some kind of gravito-optic transducer in each arm. In order to improve the shot-noise limited sensitivity, all these interferometers will use high-power lasers, in conjunction with so-called light recycling techniques. The basic idea of recycling was proposed by R. W. P. Drever (1983): it consists in building a resonant optical cavity which contains the interferometer, so that, if the losses are low and if the cavity is kept on resonance with the incoming monochromatic light, there is a power build-up which results in a reduction of the shot noise. This can be realized in different ways, depending on the geometry of the gravito-optic transducer (delay line or Fabry-Perot)." @default.
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- W1666589112 date "1991-07-25" @default.
- W1666589112 modified "2023-09-23" @default.
- W1666589112 title "Advanced techniques: recycling and squeezing" @default.
- W1666589112 doi "https://doi.org/10.1017/cbo9780511600104.017" @default.
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