Gravitational-Wave Antenna Design to Detect Random Gravitational Waves
- 15 August 1973
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 8 (4) , 1030-1035
- https://doi.org/10.1103/physrevd.8.1030
Abstract
A design is proposed for an antenna system capable of detecting random gravitational waves and separating their effects from random fluctuations in the antenna. The strongest known signal should be the random signal from all of the binary stars in the galaxy. This design may allow one to penetrate the background noise of the Earth itself and recover this signal.Keywords
This publication has 7 references indexed in Scilit:
- Upper Limit on the Gravitational Flux Reaching the Earth from the Crab PulsarPhysical Review D, 1972
- Observations of long-period (10-100 Sec) seismic noise at several worldwide locationsJournal of Geophysical Research, 1972
- A Positive Signature for the Recognition of Gravitational RadiationNature Physical Science, 1972
- Operation of LaCoste and Romberg Gravimeter at sensitivity approaching the thermal fluctuation limitsJournal of Geophysical Research, 1966
- Upper Limit for Interstellar Millicycle Gravitational RadiationNature, 1961
- Fluctuation theory in physical measurementsReports on Progress in Physics, 1953
- Extrapolation, Interpolation, and Smoothing of Stationary Time SeriesPublished by MIT Press ,1949