Publication Abstracts
Ezer and Cameron 1966
Ezer, D., and A.G.W. Cameron, 1966: Solar evolution with varying G. Can. J. Phys., 44, 593-615, doi:10.1139/p66-050.
The model-sequence calculations by the writers of early solar evolution have been extended to the case of a varying-G cosmology. In the varying-G sun there is less lithium depletion than in a constant-G sun, and the time required to burn out central hydrogen is decreased by less than the ratio of luminosities, owing to the much greater total helium production in the varying-G sun. At the present time the varying-G model has four times the 8B neutrino flux of the constant-G model, a prediction that can be subjected to an experimental check.
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BibTeX Citation
@article{ez07000g, author={Ezer, D. and Cameron, A. G. W.}, title={Solar evolution with varying G}, year={1966}, journal={Canadian Journal of Physics}, volume={44}, pages={593--615}, doi={10.1139/p66-050}, }
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RIS Citation
TY - JOUR ID - ez07000g AU - Ezer, D. AU - Cameron, A. G. W. PY - 1966 TI - Solar evolution with varying G JA - Can. J. Phys. JO - Canadian Journal of Physics VL - 44 SP - 593 EP - 615 DO - 10.1139/p66-050 ER -
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