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Conferences > CLEO_Europe > 1998 > CWF > CWF2

High power low intensity noise single frequency light sources at 1064 nm

I. Zawischa, S. Knoke, H. Zellmer, A. Tünnermann, H. Welling, O. S. Brozek, K. Danzmann, and I. Freitag

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Abstract

High power low noise lasers are needed in high precision interferometric gravitational wave detection In the GEO-600 gravitational wave detector a relative intensity noise of less than 10-8/√Hz and a frequency stability better than 10-3/√Hz will be required.

On power levels up to 2 W diode pumped non-planar monolithic Nd: YAG ring lasers (NPRO) are well known for their superior noise properties and their high potential for active stabilisation and intensity noise reduction [1].

© 1998 IEEE

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