Advanced LIGO: non-Gaussian beams

Details Advanced LIGO: non-Gaussian beams Advanced LIGO: non-Gaussian beams

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21s.867d&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 5, pp. S867-S873 (2004).

Physics

6

Scientific paper

By using non-Gaussian, flat-topped beams in the advanced gravitational wave interferometers currently being designed, one can reduce the impact on the interferometer sensitivity of a variety of fundamental disturbances (thermoelastic noise, noise in mirror coatings, thermal lensing, etc). This may make beating the standard quantum limit an achievable goal.

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