F. Guarneri, L. Pasquini, V. D'Odorico, S. Cristiani, G. Cupani, P. Di Marcantonio, J. I. González Hernández, C. J. A. P. Martins, A. Suárez Mascareño, D. Milaković, P. Molaro, M. T. Murphy, N. J. Nunes, E. Palle, F. A. Pepe, R. Rebolo, N. C. Santos, R. T. Génova-Santos, T. M. Schmidt, S. G. Sousa, A. Sozzetti, A. Trost
Abstract
Primordial abundances of light elements are sensitive to the physics of the early Universe and can directly constrain cosmological quantities, such as the baryon-to-photon ratio η10 , the baryon density, and the number of neutrino families. Deuterium is especially suited for these studies: its primordial abundance is sensitive and monotonically dependent on η10 , allowing an independent measurement of the cosmic baryon density that can be compared, for instance, against the Planck satellite data. The primordial deuterium abundance can be measured in high H I column density absorption systems towards distant quasars. We report here a new measurement, based on high-resolution ESPRESSO data, of the primordial D I abundance of a system at redshift z∼3.572 , towards PKS1937-101. Using only ESPRESSO data, we find a D /H ratio of 2.638±10−5 , while including the available UVES data improves the precision, leading to a ratio of 2.608±10−5 . The results of this analysis agree with those of the most precise existing measurements. We find that the relatively low column density of this system ( log NHI / cm−2∼18 ) introduces modelling uncertainties, which become the main contributor to the error budget.
Keywords
nuclear reactions, nucleosynthesis, abundances, quasars: absorption lines, primordial nucleosynthesis
Monthly Notices of the Royal Astronomical Society
Volume 529, Issue 2, Page 15
2024 April
