Canuto and Hsieh 1980
Canuto, V.M., and S.-H. Hsieh, 1980: Cosmological variation of G and the solar luminosity. Astrophys. J., 237, 613-615, doi:10.1086/157905.
We reexamine Teller's analysis of the effects of a varying gravitational constant G on the past solar luminosity. We show that if Newtonian gravitation is viewed as a nonrelativistic linit 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 cinluded in Teller's analysis and which change his result from L ~ G7 (found to be unacceptable) to L ~ constant independently of how G might vary with time.
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Canuto, V.M., and Hsieh, S.-H.: Cosmological variation of G and the solar luminosity, Astrophys. J., 237, 613-615, doi:10.1086/157905, 1980.
Canuto, V.M., and S.-H. Hsieh (1980), Cosmological variation of G and the solar luminosity, Astrophys. J., 237, 613-615, doi:10.1086/157905.
Canuto, V.M., and S.-H. Hsieh, 1980: Cosmological variation of G and the solar luminosity. Astrophys. J., 237, 613-615, doi:10.1086/157905.
Canuto, V.M., & Hsieh, S.-H. 1980, Astrophys. J., 237, 613, doi:10.1086/157905.
Canuto VM, Hsieh S-H. Cosmological variation of G and the solar luminosity, Astrophys J 1980;237:613-615. doi:10.1086/157905.
V.M. Canuto, S.-H. Hsieh, Astrophys. J. 237, 613-615, doi:10.1086/157905 (1980).
