The DOI matches its Crossref record; 37 of the 37 references it cites were found in a registry or an index.
Implications of WMAP Observations on Li Abundance and Stellar Evolution Models
Open accessAbstract
The Wilkinson Microwave Anisotropy Probe ( WMAP ) determination of the baryon-to-photon ratio implies, through big bang nucleosynthesis, a cosmological Li abundance larger, by a factor of 2-3, than the Li abundance plateau observed in the oldest Population II stars. It is, however, inescapable that there be a reduction by a factor of at least 1.6-2.0 of the surface Li abundance during the evolution of Population II field stars with [Fe/H] ≤ -1.5. That the observed Li should be lower than cosmologically produced Li is expected from stellar evolution models. Since at turnoff most of the Li abundance reduction is caused by gravitational settling, the presence of 6 Li in some turnoff stars is also understood. Given that the WMAP implications for Li cosmological abundance and the Li Spite plateau can be naturally explained by gravitational settling in the presence of weak turbulence, there appears little need for exotic physics as suggested by some authors. Instead, there is a need for a better understanding of turbulent transport in the radiative zones of stars. This requires simulations from first principles. Rather strict upper limits to turbulent transport are determined for the Sun and Population II stars.
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Cites
Iglesias, C. A., & Rogers, F. J. (1996) · The Astrophysical Journal · doi:10.1086/177381 · Cited by 3,020
Radiative atomic Rosseland mean opacity tables
Rogers, F. J., & Iglesias, C. A. (1992) · The Astrophysical Journal Supplement Series · doi:10.1086/191659 · Cited by 732
Radiative opacities for carbon- and oxygen-rich mixtures
Iglesias, C. A., & Rogers, F. J. (1993) · The Astrophysical Journal · doi:10.1086/172958 · Cited by 393
Coc, A., Vangioni‐Flam, E., Descouvemont, P., Adahchour, A., & Angulo, C. (2004) · The Astrophysical Journal · doi:10.1086/380121 · Cited by 370
The Spite Lithium Plateau: Ultrathin but Postprimordial
Ryan, S. G., Norris, J. E., & Beers, T. C. (1999) · The Astrophysical Journal · doi:10.1086/307769 · Cited by 297
Primordial nucleosynthesis in light of WMAP
Cyburt, R. H., Fields, B. D., & Olive, K. A. (2003) · Physics Letters B · doi:10.1016/j.physletb.2003.06.026 · Cited by 292
The Evolution of AmFm Stars, Abundance Anomalies, and Turbulent Transport
Richer, J., Michaud, G., & Turcotte, S. (2000) · The Astrophysical Journal · doi:10.1086/308274 · Cited by 270
Self-citationConsistent Solar Evolution Model Including Diffusion and Radiative Acceleration Effects
Turcotte, S., Richer, J., Michaud, G., Iglesias, C. A., & Rogers, F. J. (1998) · The Astrophysical Journal · doi:10.1086/306055 · Cited by 234
Self-citationPinsonneault, M. H., Deliyannis, C. P., & Demarque, P. (1992) · The Astrophysical Journal Supplement Series · doi:10.1086/191624 · Cited by 223
The primordial lithium abundance from extreme subdwarfs: New observations
Thorburn, J. A. (1994) · The Astrophysical Journal · doi:10.1086/173650 · Cited by 209
Cited by
Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
Spergel, D. N., Bean, R., Dore, O., Nolta, M. R., Bennett, C. L., Dunkley, J., Hinshaw, G., Jarosik, N., Komatsu, E., Page, L., et al. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513700 · Cited by 6,778
Dunkley, J., Komatsu, E., Nolta, M. R., Spergel, D. N., Larson, D., Hinshaw, G., Page, L., Bennett, C. L., Gold, B., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/306 · Cited by 1,787
Primordial nucleosynthesis: From precision cosmology to fundamental physics
Iocco, F., Mangano, G., Miele, G., Pisanti, O., & Serpico, P. D. (2009) · Physics Reports · doi:10.1016/j.physrep.2009.02.002 · Cited by 472
Precision big bang nucleosynthesis with improved Helium-4 predictions
Pitrou, C., Coc, A., Uzan, J.-P., & Vangioni, E. (2018) · Physics Reports · doi:10.1016/j.physrep.2018.04.005 · Cited by 440
Sbordone, L., Bonifacio, P., Caffau, E., Ludwig, H.-G., Behara, N. T., González Hernández, J. I., Steffen, M., Cayrel, R., Freytag, B., Van’t Veer, C., et al. (2010) · Astronomy & Astrophysics · doi:10.1051/0004-6361/200913282 · Cited by 425
Metadata
- Authors
- Richard, O., Michaud, G., & Richer, J.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2005-01-20
- Volume
- 619
- Issue
- 1
- Pages
- 538-548
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2046386183
- Cited by
- 271
- References
- 37
- FWCI
- 9.96
- Type
- journal article
- Language
- en
- Open access
- bronze
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