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4–9 Sept 2022
CERN
Europe/Zurich timezone

Precision Deuterium in Big Bang Nucleosynthesis: the Critical Role of Nuclear Reactions

6 Sept 2022, 18:00
3h
61/1-201 - Pas perdus - Not a meeting room - (CERN)

61/1-201 - Pas perdus - Not a meeting room -

CERN

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Speaker

Tsung-Han Yeh (University of Illinois Urbana-Champaign)

Description

Big Bang Nucleosynthesis (BBN) accounts for the cosmic origin of the lightest elements, and deuterium (D/H) plays a key role in probing the physics of the early universe. The simplicity of BBN theory allows for few-percent-level precision of D/H prediction, which is not normally possible in nuclear astrophysics. Under such precision, the comparison between predicted and observed primordial D/H not only provides a crucial test of the standard cosmology but also hints at new physics. The push to further improve this precision brings its own challenges and rewards: sharpening the power of BBN constraints on new physics.

The nuclear uncertainties of deuterium destruction reactions now block our way to a better D/H prediction. The reactions d(p,γ)3He, d(d,n)3He, and d(d,p)t are known to dominate the D/H theory error budget. Recent cross section measurements from LUNA significantly reduced the uncertainty of d(p,γ)3He, and the state-of-the-art D/H theory error is 3%. However, this excellent theory uncertainty still falls behind the observed counterpart; precision measurements of the primordial D/H from high redshift quasar absorption systems in the past several years have contributed to an impressive 1% error. The future improvement of D/H prediction relies on new precision measurements of d(d,n)3He and d(d,p)t at BBN energies. Moreover, ab initio theory cross section for d(p,γ)3He mismatches the precise LUNA data while agreeing with other datasets outside the BBN range. Additional theory study for d(p,γ)3He cross section is also needed to understand such a puzzling discrepancy.

Author

Tsung-Han Yeh (University of Illinois Urbana-Champaign)

Presentation materials