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Constraints on Dark Matter from Primordial Nucleosynthesis
Published online by Cambridge University Press: 04 August 2017
Abstract
Primordial nucleosynthesis which is responsible for the formation of the lightest elements (D, 3He, 4He and 7Li) provides a unique way to determine the present baryon density pB in the Universe and therefore the corresponding cosmological parameter ΩB. After a brief summary of the relevant abundance determinations and of the consequences of the Standard Big Bang nucleosynthesis, it is argued that one needs to call for specific models of chemical evolution of the Galaxy in order to reconcile the observations with the predictions of this model. In this context the predicted values for ΩB should range from 4 10−3 to 6 10−2. These values are significantly lower than those deduced from current M/L determinations.
- Type
- Review Paper
- Information
- Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 499 - 523
- Copyright
- Copyright © Reidel 1987