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Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS

Semenaite, Agne; Sánchez, Ariel G; Pezzotta, Andrea; Hou, Jiamin; Scoccimarro, Roman; Eggemeier, Alexander; Crocce, Martin; Chuang, Chia-Hsun; Smith, Alexander; Zhao, Cheng; Brownstein, Joel R; Rossi, Graziano; Schneider, Donald P

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Authors

Agne Semenaite

Ariel G Sánchez

Andrea Pezzotta

Jiamin Hou

Roman Scoccimarro

Alexander Eggemeier

Martin Crocce

Chia-Hsun Chuang

Alexander Smith

Cheng Zhao

Joel R Brownstein

Graziano Rossi

Donald P Schneider



Abstract

We present the analysis of the full shape of anisotropic clustering measurement from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) quasar sample together with the combined galaxy sample from the Baryon Oscillation Spectroscopic Survey (BOSS), re-analysed using an updated recipe for the non-linear matter power spectrum and the non-local bias parameters. We obtain constraints for flat Lambda cold dark matter cosmologies, focusing on the cosmological parameters that are independent of the Hubble parameter h. Our recovered value for the Root Mean Square (RMS) linear perturbation theory variance as measured on the scale of 12Mpc is σ12 = 0.805 ± 0.049, while using the traditional reference scale of 8h−1Mpc gives σ8 = 0.815 ± 0.044. We quantify the agreement between our measurements and the latest cosmic microwave background data from Planck using the suspiciousness metric, and find them to be consistent within 0.64 ± 0.03σ. Combining our clustering constraints with the 3 × 2pt data sample from the Dark Energy Survey Year 1 release slightly degrades this agreement to the level of 1.54 ± 0.08σ, while still showing an overall consistency with Planck. We furthermore study the effect of imposing a Planck – like prior on the parameters that define the shape of the linear matter power spectrum, and find significantly tighter constraints on the parameters that control the evolution of density fluctuations. In particular, the combination of low-redshift data sets prefers a value of the physical dark energy density ωDE = 0.335 ± 0.011, which is 1.7σ higher than the one preferred by Planck.

Citation

Semenaite, A., Sánchez, A. G., Pezzotta, A., Hou, J., Scoccimarro, R., Eggemeier, A., Crocce, M., Chuang, C.-H., Smith, A., Zhao, C., Brownstein, J. R., Rossi, G., & Schneider, D. P. (2022). Cosmological implications of the full shape of anisotropic clustering measurements in BOSS and eBOSS. Monthly Notices of the Royal Astronomical Society, 512(4), 5657-5670. https://doi.org/10.1093/mnras/stac829

Journal Article Type Article
Acceptance Date Mar 17, 2022
Online Publication Date Mar 24, 2022
Publication Date 2022-06
Deposit Date Jun 28, 2022
Publicly Available Date Jun 28, 2022
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 512
Issue 4
Pages 5657-5670
DOI https://doi.org/10.1093/mnras/stac829
Public URL https://durham-repository.worktribe.com/output/1202957

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
© The Author(s) 2022. Published by Oxford University Press on behalf of Royal Astronomical Society.
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.






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