A Quasi-Relativistic Theory of Gravitation

Details A Quasi-Relativistic Theory of Gravitation A Quasi-Relativistic Theory of Gravitation

Feb 1953

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1953phrv...89..587m&link_type=abstract

Physical Review, vol. 89, Issue 3, pp. 587-590

Physics

Scientific paper

Rays of gravitons, as well as rays of photons in a gravitational field, have transverse vibrations, and a light ray has its velocity decreased by the presence of a gravitational ray. The decrease is twice as much when they are traveling in the same direction as when they are perpendicular (and, therefore, share one dimension of vibration rather than two). Introduction of a harmonic function for the square of the velocity of light leads to Schwarzschild's equation for, first, a light ray, and then, by way of its electromagnetic field, for a particle of matter. If the sun is moving through the ether, the action of the field is relativistic, except that the angle between the light ray and the gravitational ray is measured with respect to the ether. The acceptance of Miller's ether drift data would lead, then, to perturbations of the planets, including the major part of that observed in the nodes of Venus.

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