Physics
Scientific paper
Apr 1969
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrv..180.1293n&link_type=abstract
Physical Review, vol. 180, Issue 5, pp. 1293-1298
Physics
24
Scientific paper
The Einstein gravitational theory and the Brans-Dicke gravitational theory are investigated for the gravitational-to-inertial mass ratio (mgmi) they yield for massive systems. We examine models for stars in equilibrium but undergoing rotation or containing electromagnetic radiation. General conditions on the space-time metric of many mass sources are obtained which lead to mgmi=1 for the massive systems. It is found that mgmi≠1 for a nonrotating star in the Brans-Dicke theory. The violation is of order 10-6 for the Sun. In the Brans-Dicke theory there are also contributions to mgmi≠1 due to the radiation content of a star. This violation is of order (radiation energy)/(stellar mass), yielding a correction of about 10-8 for the Sun.
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