Tinto, Massimo ; Dhurandhar, Sanjeev (1989) Astronomical observations with a network of detectors of gravitational waves. II. Solution to the four and three detector problem Monthly Notices of the Royal Astronomical Society, 236 . pp. 621-627. ISSN 0035-8711
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Official URL: http://onlinelibrary.wiley.com/journal/10.1111/%28...
Abstract
The inverse problem in the theory of gravitational wave detection is solved with a network of three or four detectors in the same location for the case in which the gravitational-wave signal is a burst with arbitrary polarization. The tensorial and spinorial properties of the wave and detector are reviewed and the solutions for the direction and the two amplitudes of the wave burst are presented. The method uses the mathematical framework of Dhurandhar and Tinto (1988).
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to John Wiley and Sons. |
| ID Code: | 87719 |
| Deposited On: | 21 Mar 2012 09:55 |
| Last Modified: | 21 Mar 2012 09:55 |
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