Concepts for third generation Gravitational Wave detectors
- Document #:
- LIGO-G1000659-v3
- Document type:
- G - Presentations (eg Graphics)
Other Versions:
- Abstract:
- esearch has started on design options for third-generation GW observatories, aiming for a sensitivity about 100 times better than first-generation instruments. In addition to the improved sensitivity, a key feature of third generation observatories will be their strongly expanded bandwidth, covering the range from 10 kHz down to frequencies as low as about 1 Hz. This talk will give an overview of innovative concepts and interferometry techniques currently considered for realising the demanding sensitivity targets of these instruments.
- Files in Document:
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- Hild_Lisa2010_final.pdf (file is not accessible)
- Topics:
- Authors:
- Keywords:
- ET third generation xylophone sensitivity studies quantum noise,
- Notes and Changes:
- Added three slides on the Science Targets of third generation GWD
- Publication Information:
- Slides for LISA Symposium, Stanford, June 2010