Abstract
We present a detailed reexamination of primordial big-bang nucleosynthesis (BBN), concentrating on the data for the main nuclear reactions leading to the production of 7Li, 3He, and D, and on the neutron half-life, relevant for 4He production. The new values for reaction rates and uncertainties are then used as input in a Monte Carlo analysis of big bang nucleosynthesis of light elements. This allows us to attach confidence levels to the predictions of the standard BBN model.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 47-59 |
| Number of pages | 13 |
| Journal | Astrophysical Journal |
| Volume | 358 |
| Issue number | 1 |
| State | Published - Jul 20 1990 |
| Externally published | Yes |
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Keywords
- Abundances
- Early universe
- Nucleosynthesis
ASJC Scopus subject areas
- Space and Planetary Science
Cite this
Big bang nucleosynthesis : Predictions and uncertainties. / Krauss, Lawrence; Romanelli, Paul.
In: Astrophysical Journal, Vol. 358, No. 1, 20.07.1990, p. 47-59.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Big bang nucleosynthesis
T2 - Predictions and uncertainties
AU - Krauss, Lawrence
AU - Romanelli, Paul
PY - 1990/7/20
Y1 - 1990/7/20
N2 - We present a detailed reexamination of primordial big-bang nucleosynthesis (BBN), concentrating on the data for the main nuclear reactions leading to the production of 7Li, 3He, and D, and on the neutron half-life, relevant for 4He production. The new values for reaction rates and uncertainties are then used as input in a Monte Carlo analysis of big bang nucleosynthesis of light elements. This allows us to attach confidence levels to the predictions of the standard BBN model.
AB - We present a detailed reexamination of primordial big-bang nucleosynthesis (BBN), concentrating on the data for the main nuclear reactions leading to the production of 7Li, 3He, and D, and on the neutron half-life, relevant for 4He production. The new values for reaction rates and uncertainties are then used as input in a Monte Carlo analysis of big bang nucleosynthesis of light elements. This allows us to attach confidence levels to the predictions of the standard BBN model.
KW - Abundances
KW - Early universe
KW - Nucleosynthesis
UR - http://www.scopus.com/inward/record.url?scp=0002045867&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0002045867&partnerID=8YFLogxK
M3 - Article
VL - 358
SP - 47
EP - 59
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
ER -