Cosmologies with variable gravitational constant

Details Cosmologies with variable gravitational constant Cosmologies with variable gravitational constant

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983foph...13..311n&link_type=abstract

Foundations of Physics, Volume 13, Issue 3, pp.311-323

Physics

7

Scientific paper

In 1937 Dirac presented an argument, based on the socalled large dimensionless numbers, which led him to the conclusion that the Newtonian gravitational constant G changes with epoch. Towards the end of the last century Ernst Mach had given plausible arguments to link the property of inertia of matter to the large scale structure of the universe. Mach's principle also leads to cosmological models with a variable gravitational constant. Three cosmologies which predict a variable G are discussed in this paper both from theoretical and observational points of view.

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