Four basic solar and stellar tests of cosmologies with variable past G and macroscopic masses

Details Four basic solar and stellar tests of cosmologies with variable past G and macroscopic masses Four basic solar and stellar tests of cosmologies with variable past G and macroscopic masses

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..359m&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 3, Apr. 1977, p. 359-367.

Astronomy and Astrophysics

Astrophysics

30

Cosmology, Gravitational Constant, Neutrinos, Stellar Evolution, Stellar Mass, Stellar Models, Mass Distribution, Open Clusters, Solar Corpuscular Radiation, Solar Flux Density, Time Functions

Scientific paper

An attempt is made to report on several tests of Dirac's cosmologies with variable G and constant macroscopic mass (1938), with variable G and additive creation (1974), and with variable G and multiplicative creation (1974). The tests involve evolutionary models of the sun with different hydrogen contents, evolutionary tracks and isochrones for stellar models of different masses, isochrones for the old open star cluster M67, the solar neutrino flux, and changes in earth's surface temperature due to solar variations. It is found that the cosmologies with constant macroscopic mass and additive creation yield results that are inconsistent with observations, but the multiplicative-creation theory gives results that are in extremely good agreement with reality. It is suggested that further tests be carried out to determine whether the extraordinary agreement of the multiplicative-creation results with observational data is a purely random effect or is of any physical significance.

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