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Bounds Upon Graviton Mass – Using the Difference Between Graviton Propagation Speed and HFGW Transit Speed to Observe Post-Newtonian Corrections to Gravitational Potential Fields: Updated to Take Into Account Early Universe Cosmology

The author presents a post-Newtonian approximation based upon an earlier argument in a paper by Clifford Will as to Yukawa revisions of gravitational potentials, in part initiated by gravitons having explicit mass dependence in their Compton wave length. Prior work with Clifford Will’s idea was stymied by the application to binary stars and other such astrophysical objects, with non-useful frequencies topping off near 100 Hertz, thereby rendering Yukawa modifications of Gravity due to gravitons effectively an experimental curiosity which was not testable with any known physics equipment. This work improves on those results. Futhermore we argue in favor of both a non zero initial radius of the universe, using Kenneth Kauthman’s work and also try to make the case for a non zero graviton mass. We use Salvoy’s document of 1983 to argue in favor of both a non zero initial radius of the universe, and non zero graviton mass ( heavy gravitons). We claim that a non-zero initial radius (of the universe) supports the massive graviton hypothesis. Which is the main point of our document. Also Gravitinos in the Electroweak era, all 10^8 10 to 10^ 12 of them have an (almost) invariant energy from the beginning of cosmology. This invariant energy constitutes an initial energy value at the start of the universe which can be used to obtain, at the onset of inflation Kauffman’s lower bound to a non zero initial radius of the universe