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Phys. Rev. Lett. 82, 4176–4179 (1999)

Sharpening the Predictions of Big-Bang Nucleosynthesis

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Scott Burles1, Kenneth M. Nollett2, James W. Truran1, and Michael S. Turner1,2,3
1Department of Astronomy & Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433
2Department of Physics, The University of Chicago, Chicago, Illinois 60637-1433
3NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500

Received 14 January 1999; published in the issue dated 24 May 1999

We have reexamined the nuclear inputs to big-bang nucleosynthesis using Monte Carlo realization of the cross-section data to directly estimate theoretical uncertainties for the yields of D, 3He, and 7Li. Our results indicate that previous estimates of the uncertainties were too large by a factor of 2. Using the Burles–Tytler deuterium measurement, we infer a baryon density ΩBh2 = 0.019±0.0024, predict a primeval 4He mass fraction YP = 0.246±0.0014, and obtain a limit to the equivalent number of neutrino species Nν<3.20 (all at 95% C.L.). We also identify key reactions and the energies, where improved data would allow further progress.

© 1999 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.82.4176
DOI:
10.1103/PhysRevLett.82.4176
PACS:
26.35.+c, 98.80.Ft