Response of a Gravitational-Wave Antenna to a Polarized Source

Physics

Scientific paper

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Scientific paper

The response of a gravitational wave antenna to linear, mixed, and
randomly polarized sources is studied as a function of sidereal time,
source coordinates, and antenna location and orientation. We find that
the gravitational signals reported by Weber cannot be highly polarized
tensor radiation coming from a single source at the Galactic nucleus.

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