Does the Standard Hot-Big-Bang Model Explain the Primordial Abundances of Helium and Deuterium?
- 18 January 1982
- journal article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 48 (3) , 209-212
- https://doi.org/10.1103/physrevlett.48.209
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Big-bang nucleosynthesis as a probe of cosmology and particle physicsThe Astrophysical Journal, 1981
- Stecker RespondsPhysical Review Letters, 1981
- Comment on the Consistency of the Standard Model of Primordial NucleosynthesisPhysical Review Letters, 1981
- Nuclear Abundances and Evolution of the Interstellar MediumAnnual Review of Astronomy and Astrophysics, 1980
- Distorted radio sources in Abell 2255 - Evidence of intergalactic gas 2.5 to 5 megaparsecs from the cluster centerThe Astrophysical Journal, 1980
- Helium Synthesis, Neutrino Flavors, and Cosmological ImplicationsPhysical Review Letters, 1980
- Spectrum of the Cosmic Background RadiationPhysical Review Letters, 1979
- Constraints on cosmology and neutrino physics from big bang nucleosynthesisThe Astrophysical Journal, 1979
- On the Synthesis of Elements at Very High TemperaturesThe Astrophysical Journal, 1967
- Primordial Helium Abundance and the Primordial Fireball. IIThe Astrophysical Journal, 1966