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Results from the Stanford 10 m Sagnac interferometer

Peter T Beyersdorf, Robert L Byer and Martin M Fejer

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The design of a 10 m all-reflective prototype Sagnac interferometer with suspended optics is described and the experimental results are presented. It uses a polarization scheme to allow detection of the dark fringe on the symmetric port of the beamsplitter for optimal interference contrast. The necessary low-frequency response of the interferometer requires delay lines in the arms. To deal with the noise introduced by scattered light in the delay lines, a laser frequency sweep frequency shifts the scattered light so that it does not produce noise near zero frequency. This results in a shot-noise-limited phase sensitivity of Δphi = 1.6 × 10−9 rad Hz−1/2 at frequencies as low as 200 Hz. Scaling this prototype to several kilometres with kilowatts of circulating power requires several technical improvements in high-power solid-state lasers, second harmonic generation and the fabrication of large mirrors, which are likely to be made in the next 10 years.


PACS

04.80.Nn Gravitational wave detectors and experiments

05.40.Ca Noise

07.60.Ly Interferometers

42.79.Fm Reflectors, beam splitters, and deflectors

MSC

83C35 Gravitational waves

Subjects

Instrumentation and measurement

Optics, quantum optics and lasers

Gravitation and cosmology

Statistical physics and nonlinear systems

Dates

Issue 7 (7 April 2002)

Received 29 October 2001, in final form 18 January 2002

Published 14 March 2002



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