The detection of gravitational radiation

Details The detection of gravitational radiation The detection of gravitational radiation

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.283..131w&link_type=abstract

In ESA, Space Science and Fundamental Physics p 131-139 (SEE N89-11638 02-88)

Physics

Antenna Design, Gravitational Wave Antennas, Gravitational Waves, Radiation Counters, Resonance, Satellite Tracking, Sensitivity, Signal To Noise Ratios, Temperature Effects

Scientific paper

The strain in space caused by gravitational radiation passing the solar system is extremely small, about 10-21. Experimental work has been going on for more than 20 years to develop antennas with sufficiently high sensitivities to detect such weak signals. The two most investigated possibilities - bar detectors and beam detectors - are described, and the present state of the art and future prospects are outlined.

Affiliated with

Also associated with

No associations

Rating

The detection of gravitational radiation 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 The detection of gravitational radiation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The detection of gravitational radiation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-854553