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Cited by 549

The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.

One Percent Determination of the Primordial Deuterium Abundance*

Open access
Cooke, Ryan J., Pettini, Max, Steidel, Charles C.·2018·The Astrophysical Journal

Abstract

We report a reanalysis of a near-pristine absorption system, located at a redshift toward the quasar Q1243+307, based on the combination of archival and new data obtained with the HIRES echelle spectrograph on the Keck telescope. This absorption system, which has an oxygen abundance [O/H] = −2.769 ± 0.028 (≃1/600 of the solar abundance), is among the lowest metallicity systems currently known where a precise measurement of the deuterium abundance is afforded. Our detailed analysis of this system concludes, on the basis of eight D i absorption lines, that the deuterium abundance of this gas cloud is , which is in very good agreement with the results previously reported by Kirkman et al., but with an improvement on the precision of this single measurement by a factor of ∼3.5. Combining this new estimate with our previous sample of six high precision and homogeneously analyzed D/H measurements, we deduce that the primordial deuterium abundance is or, expressed as a linear quantity, this value corresponds to a one percent determination of the primordial deuterium abundance. Combining our result with a big bang nucleosynthesis (BBN) calculation that uses the latest nuclear physics input, we find that the baryon density derived from BBN agrees to within 2 σ of the latest results from the Planck cosmic microwave background data.

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Metadata

Authors
Cooke, R. J., Pettini, M., & Steidel, C. C.
Venue
The Astrophysical Journal
Published
2018-03-10
Volume
855
Issue
2
Pages
102
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2766792342
Cited by
549
References
6
FWCI
28.28
Type
journal article
Language
en
Open access
bronze

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