Published March 15, 2006
| Published
Journal Article
Open
Correlation analysis of stochastic gravitational wave background around 0.1–1 Hz
- Creators
- Seto, Naoki
Chicago
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Abstract
We discuss prospects for direct measurement of stochastic gravitational wave background around 0.1–1 Hz with future space missions. It is assumed to use correlation analysis technique with the optimal time-delay-interferometry (TDI) variables for two sets of LISA-type interferometers. The signal to noise for detection of the background and the estimation errors for its basic parameters (amplitude, spectral index) are evaluated for proposed missions.
Additional Information
© 2006 The American Physical Society. (Received 17 January 2006; published 1 March 2006) The author thanks S. Kawamura and S. Phinney for valuable discussions. He also thanks N. Cornish for discussions on astrophysical foreground, C. Cutler for helpful conversations on the noise curves of BBO, and J. Yokoyama for directing his interest to this research through a collaboration.Attached Files
Published - SETprd06b.pdf
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Additional details
- Eprint ID
- 6319
- Resolver ID
- CaltechAUTHORS:SETprd06b
- Created
-
2006-12-01Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Caltech groups
- LIGO