LIGO laser intensity noise suppression

Details LIGO laser intensity noise suppression LIGO laser intensity noise suppression

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21s.481n&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 5, pp. S481-S485 (2004).

Physics

4

Scientific paper

In order to meet the strain sensitivity requirements of the Laser Interferometer Gravitational Wave Observatory (LIGO), the laser amplitude noise must be reduced to a level of 1 × 10-8 δP/P, in the bandwidth between 40 and 100 Hz, before injection into the interferometer. This paper describes the control system implemented to meet this goal.

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