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

  author={Ezer, D. and Cameron, A. G. W.},
  title={Solar evolution with varying G},
  journal={Can. J. Phys.},

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RIS Citation

ID  - ez07000g
AU  - Ezer, D.
AU  - Cameron, A. G. W.
PY  - 1966
TI  - Solar evolution with varying G
JA  - Can. J. Phys.
VL  - 44
SP  - 593
EP  - 615
DO  - 10.1139/p66-050
ER  -

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