Seto, Naoki (2006) Correlation analysis of stochastic gravitational wave background around 0.1–1 Hz. Physical Review D, 73 (6). Art. No. 063001. ISSN 2470-0010. doi:10.1103/PhysRevD.73.063001. https://resolver.caltech.edu/CaltechAUTHORS:SETprd06b
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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.
| Item Type: | Article | ||||||
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| 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. | ||||||
| Group: | LIGO | ||||||
| Subject Keywords: | gravitational wave detectors; gravitational waves; cosmology; light interferometers | ||||||
| Issue or Number: | 6 | ||||||
| DOI: | 10.1103/PhysRevD.73.063001 | ||||||
| Record Number: | CaltechAUTHORS:SETprd06b | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:SETprd06b | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 6319 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Archive Administrator | ||||||
| Deposited On: | 01 Dec 2006 | ||||||
| Last Modified: | 08 Nov 2021 20:32 |
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