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Radio interferometric tests of general relativity

Published online by Cambridge University Press:  01 October 2007

E. B. Fomalont
Affiliation:
National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA email: efomalon@nrao.edu
S. Kopeikin
Affiliation:
Dept. of Physics and Astronomy, University of Missouri, Columbia, MO 65211, USA email: kopeikins@missouri.edu
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Abstract

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Since VLBI techniques produce a microarcsecond positional accuracy of celestial objects, tests of GR using radio sources as probes of a gravitational field have been made. We present the results from two recent tests using the VLBA: in 2005, the measurement of the classical solar deflection; and in 2002, the measurement of the retarded gravitational deflection associated with Jupiter. The deflection experiment measured γ to an accuracy of 3 × 10−4; the Jupiter experiment measured the retarded term to 20% accuracy. The controversy over the interpretation of the retarded term is summarized.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Asada, H. 2002, ApJ, 574, L69CrossRefGoogle Scholar
Carlip, S. 2004, Class. Quant. Grav., 21, 3803 (arXiv:gr-qc/0403060v3)CrossRefGoogle Scholar
Fomalont, E. B., 2003, Future Directions in High Resolution Astronomy, Ed. Romney, J. D. and Reid, M. J., Socorro, NM, p55Google Scholar
Fomalont, E. B. & Kopeikin, S. M. 2003, ApJ, 598, 704CrossRefGoogle Scholar
Kopeikin, S. M. & Fomalont, E. B. 2007, Gen. Rel. and Grav., 39, 1583 (arXiv:gr-qcd/0510077v4)CrossRefGoogle Scholar
Stuart, S. 2004, Int. J. Mod. Phys., D13, 1753.Google Scholar
Treuhaft, R. N. & Lowe, S. T. 1991, AJ, 102, 1879CrossRefGoogle Scholar
Will, C. M., 2003, ApJ, 590, 683CrossRefGoogle Scholar