Median statistics analysis of deuterium abundance measurements and spatial curvature constraints

dc.contributor.authorPenton, J.
dc.contributor.authorPeyton, J.
dc.contributor.authorZahoor, A.
dc.contributor.authorRatra, B.
dc.date.accessioned2026-02-05T09:30:53Z
dc.date.issued2018
dc.description.abstractZavarygin et al. compiled a list of 15 deuterium abundance measurements; two were discarded because the remaining 13 measurements are then consistent with Gaussianity. Those authors found that the weighted-mean baryon density (?<inf>b</inf>h2) determined from the 13 measurements is mildly discrepant (1.6?) with that determined from the Planck 2015 cosmic microwave background anisotropy data in a flat cosmogony. We find that a median statistic central estimate of ?<inf>b</inf>h2 from all 15 deuterium abundance measurements is a more accurate estimate; is very consistent with ?<inf>b</inf>h2 estimated from Planck 2015 data in a flat cosmogony, but is about 2? lower than that found in a closed cosmogonical model from the Planck 2015 data. © 2018. The Astronomical Society of the Pacific. All rights reserved.
dc.identifier.citationPublications of the Astronomical Society of the Pacific, 2018, 130, 993, pp. -
dc.identifier.issn46280
dc.identifier.urihttps://doi.org/10.1088/1538-3873/aadf75
dc.identifier.urihttps://idr.nitk.ac.in/handle/123456789/24943
dc.publisherInstitute of Physics Publishing subscriptions@press.uchicago.edu
dc.subject(Cosmology:) cosmological parameters
dc.subject(Cosmology:) primordial nucleosynthesis
dc.subjectMethods: data analysis
dc.titleMedian statistics analysis of deuterium abundance measurements and spatial curvature constraints

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