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Big-bang nucleosynthesis enters the precision era
Open accessAbstract
The last parameter of big-bang nucleosynthesis, the density of ordinary matter (baryons), is being pinned down by measurements of the deuterium abundance in high-redshift hydrogen clouds. When it is, the primeval abundances of the light elements D, ${}^{3}\mathrm{He},$ ${}^{7}\mathrm{Li},$ and ${}^{4}\mathrm{He}$ will be fixed. The first three will then become ``tracers'' in the study of Galactic and stellar chemical evolution. A precision determination of the ${}^{4}\mathrm{He}$ abundance will allow an important consistency test of big-bang nucleosynthesis and will sharpen nucleosynthesis as a probe of fundamental physics, e.g., the bound to the number of light neutrino species. An independent consistency test is on the horizon: a high-precision determination of the baryon density from measurements of the fluctuations of the cosmic background radiation temperature.
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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 [17]
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Tytler, D., O’Meara, J. M., Suzuki, N., & Lubin, D. (2000) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/s0920-5632(00)00721-0 · Cited by 1
Hunting for Dark Matter particles with new detectors
Angloher, G., & Jochum, J. (2005) · Die Naturwissenschaften · doi:10.1007/s00114-004-0587-8 · Cited by 1
“By measuring the abundance of light elements in the universe one finds that the absolute amount of baryonic matter corresponds to only about 5% of the critical density (Wbar~0.05) (Schramm and Turner 1998).”
BackgroundInfluentialMeasurements of The Primordial D/H Abundance Towards Quasars
Tytler, D., O’Meara, J. M., Suzuki, N., Lubin, D., Burles, S. M., & Kirkman, D. (2000) · Symposium - International Astronomical Union · doi:10.1017/s0074180900166501 · Cited by 1
Cosmological constant and the fate of the DDM theory
Ćirković, M. M., & Samurović, S. (2001) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361:20010637/pdf · Cited by 1
Deciphering the Nature of Dark Matter
Sadoulet, B. (1999) · Springer eBooks · doi:10.1007/978-1-4612-1512-7_21 · Cited by 1
Vidal‐Madjar, A. (2000) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/s0920-5632(99)00834-8 · Cited by 1
Stellar streams as probes of the large-scale distribution of matter around galaxies
Varghese, A. (2011) · OpenGrey (Institut de l'Information Scientifique et Technique)
Deuterium, Lithium and the Density of the Universe
Audouze, J. (1999) · Springer eBooks · doi:10.1007/978-94-011-4213-7_4
Applications of Coulomb Breakup to Nuclear Astrophysics
Kiener, J. (2001) · Springer eBooks · doi:10.1007/978-94-010-0708-5_23
Metadata
- Authors
- Schramm, D. N., & Turner, M. S.
- Affiliations
- Fermi National Accelerator Laboratory (US)
- ORCID
- Turner, Michael S.
- Venue
- Reviews of Modern Physics
- Publisher
- American Physical Society (APS)
- Published
- 1998-01-01
- Volume
- 70
- Issue
- 1
- Pages
- 303-318
- ISSN
- 0034-6861 (ISSN-L)
- 1539-0756
- OpenAlex
- W2137076145
- Cited by
- 353
- References
- 77
- Citations by year
- 2026: 10 · 2025: 7 · 2024: 5 · 2023: 10 · 2022: 7 · 2021: 4 · 2020: 19 · 2019: 2 · 2018: 4 · 2017: 4 · 2016: 8 · 2015: 2 · 2014: 6 · 2013: 10 · 2012: 7
- FWCI
- 33.75
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Reviews of Modern Physics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Nuclear Physics
- Fermilab
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Nuclear physics research studies
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Neutrino Physics Research
- Keywords
- big bang nucleosynthesis, baryon density, deuterium abundance, primordial light element abundances, helium-4 abundance, helium-3, lithium-7, deuterium, number of light neutrino species, chemical evolution
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