An accurate determination of the Hubble constant from baryon acoustic oscillation datasets View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2015-09

AUTHORS

Cheng Cheng, QingGuo Huang

ABSTRACT

Even though the Hubble constant cannot be significantly determined just by the low-redshift Baryon Acoustic Oscillation (BAO) data, it can be tightly constrained once the high-redshift BAO data are combined. We combined BAO data from 6dFGS, BOSS DR11 clustering of galaxies, WiggleZ and z = 2.34 from BOSS DR11 quasar Lyman-α forest lines to get H0 = 68.17-1.56+1.55 km s-1 Mpc-1. In addition, we adopted the simultaneous measurements of H(z) and DA(z) from the two-dimensional two-point correlation function from BOSS DR9 CMASS sample and two-dimensional matter power spectrum from SDSS DR7 sample to obtain H0 = (68.11 ± 1.69) km s-1 Mpc-1. Finally, combining all of the BAO datasets, we conclude that H0 = (68.11 ± 0.86) km s-1 Mpc-1, a 1.3% determination. More... »

PAGES

599801

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s11433-015-5684-5

DOI

http://dx.doi.org/10.1007/s11433-015-5684-5

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1041310188


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