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.accessioned2020-03-31T08:39:19Z
dc.date.available2020-03-31T08:39:19Z
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 (?bh2) 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 ?bh2 from all 15 deuterium abundance measurements is a more accurate estimate; is very consistent with ?bh2 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.en_US
dc.identifier.citationPublications of the Astronomical Society of the Pacific, 2018, Vol.130, 993, pp.-en_US
dc.identifier.urihttps://idr.nitk.ac.in/handle/123456789/12459
dc.titleMedian statistics analysis of deuterium abundance measurements and spatial curvature constraintsen_US
dc.typeArticleen_US

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