Published August 7, 2006
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Journal Article
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Laser interferometry for the Big Bang Observer
Abstract
The Big Bang Observer is a proposed space-based gravitational-wave detector intended as a follow on mission to the Laser Interferometer Space Antenna (LISA). It is designed to detect the stochastic background of gravitational waves from the early universe. We discuss how the interferometry can be arranged between three spacecraft for this mission and what research and development on key technologies are necessary to realize this scheme.
Additional Information
Copyright © Institute of Physics and IOP Publishing Limited 2006. Received 24 January 2006, in final form 7 June 2006. Published 7 July 2006. Print publication: Issue 15 (7 August 2006). We would like to thank David Ottaway for useful discussions. This work was done under NASA grant NNG04GJ65G. This paper has been assigned LIGO Document Number LIGOP050054-00-R. A corrigendum for this article has been published in 2006 Class. Quantum Grav. 23 7361.Files
HARcqg06corr.pdf
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Additional details
- Eprint ID
- 6678
- Resolver ID
- CaltechAUTHORS:HARcqg06
- Created
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2006-12-17Created from EPrint's datestamp field
- Updated
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2022-07-12Created from EPrint's last_modified field
- Caltech groups
- TAPIR