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Primordial nucleosynthesis: theory and observations
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“The agreement between the WMAP results[15, 16, 17, 18] and the most recent analysis of the primordial deuterium abundance[46] yields”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [16]
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“8 and TB ≈ 1MeV are the effective degrees of freedom of the radiation and the temperature at the BBN era respectively [59].”
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Cohen, A. G. (1999) · Cited by 1
Metadata
- Authors
- Olive, K. A., Steigman, G., & Walker, T. P.
- Affiliations
- University of Minnesota (US)
- The Ohio State University (US)
- Corresponding author
- Olive, Keith A
- ORCID
- Olive, Keith A
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2000-08
- Volume
- 333-334
- Pages
- 389-407
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W2121134683
- Cited by
- 448
- References
- 89
- Citations by year
- 2026: 11 · 2025: 9 · 2024: 10 · 2023: 5 · 2022: 11 · 2021: 5 · 2020: 6 · 2019: 4 · 2018: 14 · 2017: 4 · 2016: 13 · 2015: 8 · 2014: 8 · 2013: 11 · 2012: 17
- FWCI
- 39.87
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physics Reports (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Neutrino Physics Research
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Nuclear physics research studies
- Keywords
- big bang nucleosynthesis, primordial abundances, baryon density, light particles, effective interaction, massless neutrinos, cosmology
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