A new, precise measurement of the primordial abundance of Deuterium

TL;DR

This paper presents a highly precise measurement of the primordial deuterium abundance using a carefully analyzed DLA system, aligning well with CMB data and reducing the need for non-standard physics.

Contribution

It introduces a new, highly accurate measurement method for (D/H)_p in a specific DLA, emphasizing comprehensive error analysis and consistency with cosmological models.

Findings

Measured (D/H)_p = (2.535 +/- 0.05) x 10^(-5)

Derived Omega_b h^2 = 0.0223 +/- 0.0009

Results agree with CMB measurements of Omega_b h^2

Abstract

The metal-poor damped Lyman alpha (DLA) system at z = 3.04984 in the QSO SDSSJ1419+0829 has near-ideal properties for an accurate determination of the primordial abundance of deuterium, (D/H)_p. We have analysed a high-quality spectrum of this object with software specifically designed to deduce the best fitting value of D/H and to assess comprehensively the random and systematic errors affecting this determination. We find (D/H)_DLA = (2.535 +/-0.05) x 10^(-5), which in turn implies Omega_b h^2 = 0.0223 +/- 0.0009, in very good agreement with Omega_b h^2 (CMB) = 0.0222 +/- 0.0004 deduced from the angular power spectrum of the cosmic microwave background. If the value in this DLA is indeed the true (D/H)_p produced by Big-Bang nucleosynthesis (BBN), there may be no need to invoke non-standard physics nor early astration of D to bring together Omega_b h^2 (BBN) and Omega_b h^2 (CMB). The scatter between most of the reported values of (D/H)_p in the literature may be due largely to unaccounted systematic errors and biases. Further progress in this area will require a homogeneous set of data comparable to those reported here and analysed in a self-consistent manner. Such an endeavour, while observationally demanding, has the potential of improving our understanding of BBN physics, including the relevant nuclear reactions, and the subsequent processing of 4He and 7Li through stars.