Gravitation Theory: Empirical Status from Solar System Experiments
- 15 December 1972
- journal article
- research article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 178 (4066) , 1157-1164
- https://doi.org/10.1126/science.178.4066.1157
Abstract
I have reviewed the historical and contemporary experiments that guide us in choosing a post-Newtonian, relativistic gravitational theory. The foundation experiments essentially constrain gravitation theory to be a metric theory in which matter couples solely to one gravitational field, the metric field, although other cosmological gravitational fields may exist. The metric field for any metric theory can be specified (for the solar system, for our present purposes) by a series of potential terms with several parameters. A variety of experiments specify (or put limits on) the numerical values of the seven parameters in the post-Newtonian metric field, and other such experiments have been planned. The empirical results, to date, yield values of the parameters that are consistent with the predictions of Einstein's general relativity.Keywords
This publication has 31 references indexed in Scilit:
- Vector-Metric Theory of GravityPhysical Review D, 1973
- A New Theory of GravityPhysical Review D, 1973
- Conservation Laws and Preferred Frames in Relativistic Gravity. I. Preferred-Frame Theories and an Extended PPN FormalismThe Astrophysical Journal, 1972
- Mercury's Perihelion Advance: Determination by RadarPhysical Review Letters, 1972
- Fourth Test of General Relativity: New Radar ResultPhysical Review Letters, 1971
- Gravitational Constant: Experimental Bound on Its Time VariationPhysical Review Letters, 1971
- Anisotropy and Polarization in the Gravitational-Radiation ExperimentsPhysical Review Letters, 1970
- Solar Oblateness and General RelativityPhysical Review Letters, 1967
- Mach's Principle and a Relativistic Theory of GravitationPhysical Review B, 1961
- On Continued Gravitational ContractionPhysical Review B, 1939