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NSR database version of May 10, 2024.

Search: Author = S.Burles

Found 4 matches.

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2001BU09      Phys.Rev. D63, 063512 (2001)

S.Burles, K.M.Nollett, M.S.Turner

What is the Big-Bang-Nucleosynthesis Prediction for the Baryon Density and How Reliable is it ?

NUCLEAR REACTIONS 2H(d, n), E(cm)=0.01-0.6 MeV; compiled, evaluated σ data. Baryon density derived from 2H/1H abundances and σ data.

doi: 10.1103/PhysRevD.63.063512
Citations: PlumX Metrics


2001BU22      Astrophys.J. 552, L1 (2001)

S.Burles, K.M.Nollett, M.S.Turner

Big Bang Nucleosynthesis Predictions for Precision Cosmology

doi: 10.1086/320251
Citations: PlumX Metrics


2000BU09      Nucl.Phys. A663-664, 861c (2000)

S.Burles

Deuterium and Big Bang Nucleosynthesis

doi: 10.1016/S0375-9474(99)00732-0
Citations: PlumX Metrics


1999BU10      Phys.Rev.Lett. 82, 4176 (1999)

S.Burles, K.M.Nollett, J.W.Truran, M.S.Turner

Sharpening the Predictions of Big-Bang Nucleosynthesis

NUCLEAR REACTIONS 1H(n, γ), 2H(p, γ), (d, p), (d, n), 3H(α, γ), (d, n), 3He(α, γ), (d, p), (n, p), 7Li(p, α), (p, n), E < 2000 keV; analyzed data. 2H, 3,4He, 7Li; deduced big-bang nucleosynthesis yields, sources of uncertainty.

doi: 10.1103/PhysRevLett.82.4176
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