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  LISA and ground-based detectors for gravitational waves: an overview

Danzmann, K., & LISA Study Team (1998). LISA and ground-based detectors for gravitational waves: an overview. In W. M. Folkner (Ed.), Laser interferometer space antenna (pp. 3-10). Woodbury, NY: American Inst. of Physics.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-5A44-4 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-5A45-2
Genre: Conference Paper

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 Creators:
Danzmann, Karsten1, Author           
LISA Study Team, Author  
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              

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 Abstract: The gravitational wave spectrum covers many decades in frequency. Sources in the audio-frequency regime above 1 Hz are accessible to ground-based detectors while sources in the low-frequency regime can only be observed from space because of the unshieldable background of local gravitational noise on the ground and because ground-based interferometers are limited in length to a few kilometers. Laser interferometry is a promising technique to observe the minute distance changes caused by gravitational waves, but the actual implementation is very different on ground and in space. An overview of LISA and other detectors will be given.

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 Dates: 1998
 Publication Status: Issued
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 Identifiers: eDoc: 372483
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Title: Second International LISA Symposium on the Detection and Observation of Gravitational Waves in Space
Place of Event: Pasadena, California
Start-/End Date: 1998-07 - 1998-07

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Title: Laser interferometer space antenna
Source Genre: Proceedings
 Creator(s):
Folkner, William M., Editor
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Publ. Info: Woodbury, NY : American Inst. of Physics
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 3 - 10 Identifier: ISBN: 1-563-96848-7

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Title: AIP conference proceedings
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Pages: - Volume / Issue: 456 Sequence Number: - Start / End Page: - Identifier: ISBN: 1-563-96848-7