Polarization resolution of LISA

Jennrich, O.; Peterseim, M.; Danzmann, K.; Schutz, B. F.

doi:10.1088/0264-9381/14/6/022

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Polarization resolution of LISA

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Danzmann, K.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Schutz, B. F.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Jennrich, O., Peterseim, M., Danzmann, K., & Schutz, B. F. (1997). Polarization resolution of LISA. Classical and Quantum Gravity, 14(6), 1525-1529. doi:10.1088/0264-9381/14/6/022.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-0F55-8

Abstract

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.