The LBT $Y_{\rm p}$ Project V: Cosmological Implications of a New Determination of Primordial $^4$He
Tsung-Han Yeh, Keith A. Olive, Brian D. Fields, Erik Aver, Richard W. Pogge, Noah S. J. Rogers, Evan D. Skillman, Miqaela K. Weller

TL;DR
This study presents the most precise measurement of primordial helium abundance, combining it with deuterium data to refine cosmological parameters and test the consistency of the Standard Model and standard cosmology.
Contribution
The paper provides the most precise primordial helium measurement and explores its implications for cosmological parameters, including baryon density and relativistic species during nucleosynthesis.
Findings
Primordial helium abundance measured as Yp=0.2458 ± 0.0013.
Cosmic baryon-to-photon ratio determined as η=(6.120 ± 0.038)×10^(-10).
Number of relativistic species during nucleosynthesis consistent with three.
Abstract
The primordial abundance of He plays a central role in big-bang nucleosynthesis (BBN) and in the cosmic microwave background (CMB). The LBT Project's new measurement of the primordial He mass fraction is the most precise determination to date. In this paper, we combine our new value with the latest primordial deuterium measurement, and assess the consequences for cosmology. For Standard BBN, where the number of light neutrino species is fixed at , the single free parameter is the cosmic baryon density; the CMB measures this independently, with results consistent with each other. Combining , D/H, BBN, and the CMB, gives the cosmic baryon-to-photon ratio , corresponding to a baryon density parameter . We then allow …
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Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Dark Matter and Cosmic Phenomena
