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Cosmological Synthesis of the Elements

Published online by Cambridge University Press:  07 February 2017

Robert V. Wagoner
Robert V. Wagoner*
Affiliation:
Dept. of Astronomy and Center for Radiophysics and Space Research, Cornell University, Ithaca, N.Y. 14850, U.S.A.cor1corresp
∗∗
*
Present address. Institute of Theoretical Physics, Dept. of Physics, Stanford University, Stanford, Calif. 94305, U.S.A.

Abstract

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The results of improved calculations of the abundances of the nuclei produced in big-bang models of the early universe are presented. In addition to the standard model, other possible universes are considered, including the recent statistical bootstrap theory of Carlitz, Frautschi, and Nahm. Some conclusions which can be drawn about the nature of the early universe, depending upon whether the observed deuterium and helium are of galactic or cosmological origin, are presented.

Type
Part III: Relic Radiation
Information
Symposium - International Astronomical Union , Volume 63: Confrontation of Cosmological Theories , 1974 , pp. 195 - 210
Copyright
Copyright © Reidel 1974 

Footnotes

∗

Supported in part by the National Science Foundation (GP-26068) at Cornell University and (GP-39178) at Stanford University.

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