We present measurements of Baryon Acoustic Oscillation
(BAO) distances used as an uncalibrated standard ruler that
determine $\Omega_{\textrm{de}}(a)$, $\Omega_k$, $\Omega_m$, and $d_{\textrm{BAO}} \equiv r_* H_0 / c$;
and BAO distances used as a calibrated standard ruler
$r_*$ that constrains a combination of $\sum m_\nu$, $h$, and $\Omega_b h^2$.
The cosmological parameters obtained in this analysis are
compared with the Review of Particle Physics, PDG 2018.
Volume 335 -
2nd World Summit: Exploring the Dark Side of the Universe (EDSU2018) -
The Cosmos as a Particle Detector
Galaxy Clustering and Baryon Acoustic Oscillations
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Pre-published on:
November 27, 2018
Published on:
December 18, 2018
Abstract
DOI: https://doi.org/10.22323/1.335.0004
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.