Cosmological variation of G and the solar luminosity

Details Cosmological variation of G and the solar luminosity Cosmological variation of G and the solar luminosity

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..613c&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, Apr. 15, 1980, p. 613-615.

Astronomy and Astrophysics

Astrophysics

10

Cosmology, Gravitational Constant, Periodic Variations, Solar Flux Density, Stellar Luminosity, Lagrange Coordinates, Newton Theory, Nonrelativistic Mechanics, Solar Temperature, Stellar Mass

Scientific paper

Teller's analysis of the effects of a varying gravitational constant G on the past solar luminosity is reexamined. It is shown that if Newtonian gravitation is viewed as a nonrelativistic limit of Einstein's theory, there exists (1) a constraint between G and the total mass M of the sun and (2) a change in the radiative energy density-temperature relation, which were not included in Teller's analysis and which change his result from L is about G to the 7th power (found to be unacceptable) to L is about constant, independently of how G might vary with time.

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