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  Gravitational wave detectors

Aufmuth, P., & Danzmann, K. (2005). Gravitational wave detectors. New Journal of Physics, 7: 202. doi:10.1088/1367-2630/7/1/202.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4F8D-8 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4F8E-6
Genre: Journal Article

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njp5_1_202.pdf (Publisher version), 2MB
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 Creators:
Aufmuth, Peter1, Author              
Danzmann, Karsten1, Author              
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              

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 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.

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Language(s): eng - English
 Dates: 2005
 Publication Status: Published in print
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Title: New Journal of Physics
Source Genre: Journal
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Pages: - Volume / Issue: 7 Sequence Number: 202 Start / End Page: - Identifier: ISSN: 1367-2630