Discriminating a gravitational wave background from instrumental noise in the LISA detector

Details Discriminating a gravitational wave background from instrumental noise in the LISA detector Discriminating a gravitational wave background from instrumental noise in the LISA detector

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvd..63b1101t&link_type=abstract

Physical Review D, vol. 63, Issue 2, id. 021101

Other

44

Gravitational Wave Detectors And Experiments, Interferometers, Gravitational Radiation Detectors, Mass Spectrometers, And Other Instrumentation And Techniques

Scientific paper

The multiple Doppler readouts available with the Laser Interferometer Space Antenna (LISA) permit simultaneous formation of several observables. All are independent of laser phase fluctuations, but have different couplings to gravitational waves and the various LISA instrumental noises. Comparison, for example, of the Michelson interferometer observable with the fully symmetric Sagnac data-type allows discrimination between a confusion-limited gravitational wave background and instrumental noise.

Affiliated with

Also associated with

No associations

Rating

Discriminating a gravitational wave background from instrumental noise in the LISA detector 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 Discriminating a gravitational wave background from instrumental noise in the LISA detector, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discriminating a gravitational wave background from instrumental noise in the LISA detector will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-904827