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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]
Citations
Cites
A Measurement of Excess Antenna Temperature at 4080 Mc/s.
Penzias, A. A., & Wilson, R. W. (1965) · The Astrophysical Journal · doi:10.1086/148307 · Cited by 2,606
The Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set
Fixsen, D. J., Cheng, E. S., Gales, J. M., Mather, J. C., Shafer, R. A., & Wright, E. L. (1996) · The Astrophysical Journal · doi:10.1086/178173 · Cited by 1,780
Fukugita, M., Hogan, C. J., & Peebles, P. J. E. (1998) · The Astrophysical Journal · doi:10.1086/306025 · Cited by 1,216
Primordial nucleosynthesis redux
Walker, T. P., Steigman, G., Kang, H.-S., Schramm, D., & Olive, K. A. (1991) · The Astrophysical Journal · doi:10.1086/170255 · Cited by 805
Self-citationThe Cosmic Baryon BudgetPreprint
Fukugita, M., Hogan, C. J., & Peebles, P. J. E. (1997) · Cited by 733
Primordial nucleosynthesis - A critical comparison of theory and observation
Yang, J., Turner, M. S., Schramm, D. N., Steigman, G., & Olive, K. A. (1984) · The Astrophysical Journal · doi:10.1086/162123 · Cited by 667
Self-citationThe primordial helium abundance from observations of extragalactic H II regions
Pagel, B. E. J., Simonson, E. A., Terlevich, R. J., & Edmunds, M. G. (1992) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/255.2.325 · Cited by 579
Big bang nucleosynthesis and physics beyond the standard model
Sarkar, S. (1996) · Reports on Progress in Physics · doi:10.1088/0034-4885/59/12/001 · Cited by 546
The primordial helium abundance from a new sample of metal-deficient blue compact galaxies
Izotov, Y. I., Thuan, T. X., & Lipovetsky, V. A. (1994) · The Astrophysical Journal · doi:10.1086/174843 · Cited by 484
The Primordial Helium Abundance: Systematic Effects and a New Determination
Izotov, Y. I., Thuan, T. X., & Lipovetsky, V. A. (1997) · The Astrophysical Journal Supplement Series · doi:10.1086/312956 · Cited by 441
Research works printed but not linked: 9
- Hubble, 1927, Proc. Natl. Acad. Sci., 71, 231
- Smoot, 1998, Eur. Phys. J. C, 3, 127
- S. Burles, K.M. Nollett, J.N. Truran, M.S. Turner, astro-ph/9901157. · arXiv
- T.P. Walker, Ph.D. Thesis, Indiana University, 1987.
- P.J. Kernan, Ph.D. Thesis, The Ohio State University, 1993.
- D. Seckel, hep-ph/9305311. · arXiv
- Vidal-Madjar, 1998, Astron. Astrophys., 338, 694
- S. Levshakov, D. Tytler, S. Burles, astro-ph/9812114. · arXiv
- Levshakov, 1998, Astron. Astrophys., 336, 29L
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Self-citationNew BBN limits on physics beyond the standard model from 4He
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Self-citationUpdated nucleosynthesis constraints on unstable relic particles
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Self-citationCosmological parameters from the first results of Boomerang
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“At high densities and temperatures, high-energy photons interact very fast with the thermal bath creating 5When facing standard ALP-less cosmology, our results are in very good agreement with standard BBN calculations obtained with the KAWANO [26] or PArthENoPE [27] codes, given the theoretical and experimental uncert…”
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Self-citationThe Cosmic Microwave Background
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An update on the big bang nucleosynthesis prediction for 7Li: the problem worsens
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Self-citationCompilation and R-matrix analysis of Big Bang nuclear reaction rates
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Olive, K. A., & Skillman, E. D. (2004) · The Astrophysical Journal · doi:10.1086/425170 · Cited by 244
“Here we are interested in the redundancies in the determination of the baryon density, B, using both the CMB and big bang nucleosynthesis (BBN; Walker et al. 1991; Sarkar 1996; Olive et al. 2000; Fields & Sarkar 2002).”
MethodSelf-citationCosmic Microwave Background Observables and Their Cosmological Implications
Hu, W., Fukugita, M., Zaldarriaga, M., & Tegmark, M. (2001) · The Astrophysical Journal · doi:10.1086/319449 · Cited by 244
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“On the other hand, if r(2)(yR) is much greater than 10−1, the expansion rate in the early Universe would be so huge that it would spoil the predictions of the primordial nucleosynthesis [108].”
BackgroundCosmic clocks, cosmic variance and cosmic averages
Wiltshire, D. L. (2007) · New Journal of Physics · doi:10.1088/1367-2630/9/10/377 · Cited by 246
Sievers, J. L., Bond, J. R., Cartwright, J. K., Contaldi, C., Mason, B., Myers, S. T., Padin, S., Pearson, T. J., Pen, U., Pogosyan, D., et al. (2003) · The Astrophysical Journal · doi:10.1086/375510 · Cited by 215
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“Analyses of Big Bang nucleosynthesis [5] imply the baryonic density Ωbh 2 ' 0.”
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Compilation and R-matrix analysis of Big Bang nuclear reaction ratesPreprint
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Review of Big Bang Nucleosynthesis and Primordial Abundances
Tytler, D., O’Meara, J. M., Suzuki, N., & Lubin, D. (2000) · Physica Scripta · doi:10.1238/physica.topical.085a00012 · Cited by 175
“[6], [7], [8], [9], [10], [11], [12] and [13], some of which are lengthy: e.”
Supersymmetric CP-violating currents and electroweak baryogenesis
Carena, M. S., Moreno, J. M., Mariano Quirós, C., Seco, M., & Wagner, C. E. M. (2001) · Nuclear Physics B · doi:10.1016/s0550-3213(01)00032-3 · Cited by 174
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“This value, after Big Bang nucleosynthesis calculations (e.g., Olive et al. 2000) is only marginally consistent (at the 2 σ level) with the best fit to cosmic microwave background (CMB) measurements (e.g., Jaffe et al. 2001).”
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“The successful calculation of the primordial lightelement abundances in the framework of the standard theory of big-bang nucleosynthesis (BBN) [1, 2, 3, 4] is among the main pillars supporting our modern understanding of the universe.”
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“…we add to the Standard Model lagrangian the following renormalizable lagrangian (other than the kinetic terms for the various new fields) ∆L = λFHS + λcFcH†S +MFFc + µS2 + h.c. (2) The doublets Fc and F have respectively hypercharge ±1/2, S is a singlet and H is the Standard Model Higgs doublet.”
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Self-citationA new approach to systematic uncertainties and self-consistency in helium abundance determinationsPreprint
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Inter-galactic Shock Acceleration and the Cosmic Gamma-ray BackgroundPreprint
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Self-citationThe impact of new d(p,γ)3 rates on Big Bang Nucleosynthesis
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Self-citationSolar neutrino constraints on the BBN production of Li
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Self-citationTime variation of the fine structure constant driven by quintessence
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Self-citation
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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