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Anisotropy and Polarization in the Gravitational-Radiation Experiments

J. Weber
Phys. Rev. Lett. 25, 180 – Published 20 July 1970
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Abstract

Large anisotropy is observed for gravitational-radiation-detector intensity as a function of sidereal time, with peaks in the direction of the galactic center and in the opposite direction consistent with 12-h antenna symmetry. The 12-h sidereal-time histograms exhibit anisotropy exceeding 6 standard deviations from the mean.

  • Received 8 September 1969

DOI:https://doi.org/10.1103/PhysRevLett.25.180

©1970 American Physical Society

Authors & Affiliations

J. Weber*

  • Institute for Advanced Study, Princeton, New Jersey 08540

  • *On leave from University of Maryland, College Park, Md. 20742.

See Also

A Fleeting Detection of Gravitational Waves

David Lindley
Phys. Rev. Focus 16, 19 (2005)

References

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Issue

Vol. 25, Iss. 3 — 20 July 1970

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