Other
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006phrvd..73l2005s&link_type=abstract
Physical Review D, vol. 73, Issue 12, id. 122005
Other
11
Gravitational Wave Detectors And Experiments, Interferometers, Modulation And Optical Transfer Functions, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques
Scientific paper
The sensitivity of next-generation gravitational-wave detectors such as Advanced LIGO and LCGT should be limited mostly by quantum noise with an expected technical progress to reduce seismic noise and thermal noise. Those detectors will employ the optical configuration of resonant-sideband-extraction that can be realized with a signal-recycling mirror added to the Fabry-Perot Michelson interferometer. While this configuration can reduce quantum noise of the detector, it can possibly increase laser frequency noise and intensity noise. The analysis of laser noise in the interferometer with the conventional configuration has been done in several papers, and we shall extend the analysis to the resonant-sideband-extraction configuration with the radiation-pressure effect included. We shall also refer to laser noise in the case we employ the so-called DC readout scheme.
Chen Yafeng
Kawamura Seiji
Mio Norikatsu
Somiya Kentaro
No associations
LandOfFree
Frequency noise and intensity noise of next-generation gravitational-wave detectors with RF/DC readout schemes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Frequency noise and intensity noise of next-generation gravitational-wave detectors with RF/DC readout schemes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Frequency noise and intensity noise of next-generation gravitational-wave detectors with RF/DC readout schemes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1476640