The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
Siddharth Satpathy, Shadab Alam, Shirley Ho, Martin White, Neta A. Bahcall, Florian Beutler, Joel R. Brownstein, Chia-Hsun Chuang, Daniel J. Eisenstein, Jan Niklas Grieb, Francisco Kitaura, Matthew D. Olmstead, Will J. Percival, Salvador Salazar-Albornoz, Ariel G. Sánchez, Hee-Jong Seo, Daniel Thomas, Jeremy L. Tinker, Rita Tojeiro
TL;DR
This study uses the CLPT-GSRSD framework to extract the linear growth rate from redshift-space distortions in the SDSS-III BOSS DR12 galaxy sample, analyzing three overlapping redshift bins. By modeling the monopole and quadrupole of the two-point correlation function via Convolution Lagrangian Perturbation Theory and Gaussian Streaming, the authors infer $f\sigma_8(z)$ along with Alcock-Paczyński parameters and distance measures, validated against MD-P mocks. The results, consistent with Planck LCDM-GR, provide robust growth-rate constraints across $0.2<z<0.75$ and demonstrate the method’s viability for gravity tests, while also contributing to the final BOSS consensus cosmology released in Alam et al. 2016. The work emphasizes the balance between exploiting quasi-linear scales for precision and avoiding strongly non-linear regimes where the model is less reliable, highlighting avenues for future small-scale RSD modeling improvements.
Abstract
We present a measurement of the linear growth rate of structure, \textit{f} from the Sloan Digital Sky Survey III (SDSS III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using Convolution Lagrangian Perturbation Theory (CLPT) with Gaussian Streaming Redshift-Space Distortions (GSRSD) to model the two point statistics of BOSS galaxies in DR12. The BOSS-DR12 dataset includes 1,198,006 massive galaxies spread over the redshift range $0.2 < z < 0.75$. These galaxy samples are categorized in three redshift bins. Using CLPT-GSRSD in our analysis of the combined sample of the three redshift bins, we report measurements of $f σ_8$ for the three redshift bins. We find $f σ_8 = 0.430 \pm 0.054$ at $z_{\rm eff} = 0.38$, $f σ_8 = 0.452 \pm 0.057$ at $z_{\rm eff} = 0.51$ and $f σ_8 = 0.457 \pm 0.052$ at $z_{\rm eff} = 0.61$. Our results are consistent with the predictions of Planck $Λ$CDM-GR. Our constraints on the growth rates of structure in the Universe at different redshifts serve as a useful probe, which can help distinguish between a model of the Universe based on dark energy and models based on modified theories of gravity. This paper is part of a set that analyses the final galaxy clustering dataset from BOSS. The measurements and likelihoods presented here are combined with others in Alam et al. 2016 to produce the final cosmological constraints from BOSS.
