Mach's principle and Yukawa-like corrections to the Newtonian potential as a bound for the mean energy density of the universe

Details Mach's principle and Yukawa-like corrections to the Newtonian potential as a bound for the mean energy density of the universe Mach's principle and Yukawa-like corrections to the Newtonian potential as a bound for the mean energy density of the universe

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.315..285m&link_type=abstract

Astrophysics and Space Science, Volume 315, Issue 1-4, pp. 285-286

Astronomy and Astrophysics

Astrophysics

Inertia, Mass Density Of The Universe, Graviton

Scientific paper

The (Newton + Yukawa)-type gravitational potential V( r)=-( γ M/ r)[1+ Aexp (- r/ B)]( γ= the gravitational constant as measured at infinity, M= the mass of the source, A, B are constants) is considered in the framework of the Sciama linear approach to Mach’s principle. The coupling constant A of the Yukawa component is found to be related to the mass density and size of the observable (causally connected) universe.

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