Physics
Scientific paper
Mar 1972
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972amjph..40..398p&link_type=abstract
American Journal of Physics, Volume 40, Issue 3, pp. 398-400 (1972).
Physics
1
Scientific paper
The nonlinearity of Einstein's gravitational equations produces three-body forces in the equations of motion. One of their consequences is that the motion of an electron around a nucleus (or a satellite around a planet) is slowed down by the existence of a distant massive body. This is the familiar gravitational red shift, which can thus be derived without invoking the equivalence principle.
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