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Gravitational wave detectors

Peter Aufmuth et al 2005 New J. Phys. 7 202   doi: 10.1088/1367-2630/7/1/202  Help

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Peter Aufmuth and Karsten Danzmann
Max-Planck-Institut für Gravitationsphysik (Albert Einstein Institut), Universität Hannover, Callinstr. 38, D-30167 Hannover, Germany
E-mail: peter.aufmuth@aei.mpg.de

Part of Focus on Spacetime 100 Years Later

Abstract. The existence of gravitational radiation is a prediction of Einstein's general theory of relativity. Gravitational waves are perturbations in the curvature of spacetime caused by accelerated masses. Since the 1960s gravitational wave detectors have been built and constantly improved. The present-day generation of resonant mass antennas and laser interferometers has reached the necessary sensitivity to detect gravitational waves from sources in the Milky Way. Within a few years, the next generation of detectors will open the field of gravitational wave astronomy.

Received 6 September 2004
Published 29 September 2005

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