Abstract
We discuss optical methods which either enhance the signal response or reduce the quantum noise in a long baseline interferometric type detector of gravitational waves. We review current progress in the science and engineering of the different techniques and consider when they may be applicable to full scale interferometers.
Original language | English |
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Pages (from-to) | 270-281 |
Number of pages | 12 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 4856 |
DOIs | |
Publication status | Published - 2002 |
Event | Gravitational - Wave Detection - Waikoloa, HI, United States Duration: 23 Aug 2002 → 25 Aug 2002 |