Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..621t&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Feb. 1, 1989, p. 621-627. Research supported by SE
Astronomy and Astrophysics
Astronomy
18
Gravitational Wave Antennas, Polarization (Waves), Nonlinearity, Radiation Detectors, Wave Equations
Scientific paper
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).
Dhurandhar Sanjeev
Tinto Massimo
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