Cosmology Results from eBOSS

The SDSS Baryon Acoustic Oscillation (BAO) and Redshift-Space Distortion (RSD) measurements reveal an uninterrupted view of the cosmos over the last 11 billion years. This composite sample is the most constraining of its kind and allows a comprehensive assessment of the cosmological model. These final measurements are broadly described in the final eBOSS press release.
Contemporaneously with the BOSS and eBOSS surveys, which have fostered the development of the BAO and RSD techniques over the last 10 years, maps of the Cosmic Microwave Background (CMB) produced by the Planck satellite have given insight into the state of the Universe as it was during the recombination era. Large weak lensing surveys such as the Dark Energy Survey (DES) have measured cosmic shear to constrain the local matter density and amplitude of fluctuations. Type Ia supernovae (SNe Ia) measurements remain the most effective way to constrain expansion history at redshifts below $z<0.3$, with some of the latest results coming from the Pantheon sample of SNe Ia.
In the final eBOSS cosmology analysis (2020) , we present the cosmological model and its observational signatures. We use the BAO and RSD data from SDSS, the Planck CMB data, SNe Ia from the Pantheon sample, and weak lensing and clustering data from DES to provide the tightest available constraints on the parameters within the standard ΛCDM model and its extensions. In the brief summary of these results presented on this web page, we denote the Planck CMB data as `CMB T&P' when no lensing is used, `CMB lens' when only the lensing is used, and `Planck' when all data are used. We refer to the DES weak lensing data as `WL' and we refer to the full DES weak lensing, galaxy-galaxy lensing, and clustering data as `DES'.
We begin with a discussion of BAO measurements in the context of the cosmic expansion history. We demonstrate that BAO are able to constrain single-parameter extensions to a ΛCDM cosmology that can not be constrained by CMB alone, and that BAO data are unique in their ability to provide robust, consistent measurements of the current expansion rate, H0. We then discuss the insight offered by RSD measurements, showing that the RSD, CMB, and weak lensing measurements present a history of structure growth that is best described by a standard ΛCDM cosmology and a GR model for gravity. Finally, we present the cosmological model that best describes the available data and how constraints on that model have advanced in the last ten years.
More details about these analyses can be found in the final eBOSS cosmology analysis (2020) , with an emphasis on the SDSS, BOSS, and eBOSS cosmology programs.


BAO and Expansion History
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RSD and Structure Growth
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Global Cosmology Constraints
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