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1997 Class. Quantum Grav. 14 1525-1529 doi: 10.1088/0264-9381/14/6/022
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Institut für Atom- und Molekülphysik, Universität Hannover, Appelstraße 2, 30167 Hannover, Germany Max-Planck-Institut für Quantenoptik, Hans-Kopfermann-Straße 1, 85748 Garching, GermanyAbstract.
We discuss LISA's ability to resolve different polarizational states of a gravitational wave with fixed frequency and amplitude. Assuming a binary as the source of the gravitational wave, its orientation is connected with the polarization of the gravitational wave emitted. Using methods of signal processing, we calculate the 1-
uncertainty range for measuring the orientation of the source.
PACS numbers: 9780G, 9585S, 0480N, 9555Y
Print publication: Issue 6 (June 1997) |
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