The cosmological bulk flow: consistency with $\Lambda$CDM and $z\approx 0$ constraints on $\sigma_8$ and $\gamma$
Adi Nusser, Marc Davis

TL;DR
This paper estimates the cosmic bulk flow using the SFI++ Tully-Fisher catalog, finds results consistent with the $ m f ext{Lambda}CDM$ model, and constrains cosmological parameters, ruling out some alternative models.
Contribution
It introduces the extsc{Ace} method for reconstructing bulk flow from peculiar velocity data, providing robust constraints on cosmological parameters.
Findings
Bulk flow measurements are consistent with $ m f ext{Lambda}CDM$ predictions.
Derived constraints on $oldsymbol{\sigma_8}$, $oldsymbol{\Omega_m}$, and $oldsymbol{\gamma}$.
Rules out DGP models at over 99 ext{\%} confidence level.
Abstract
We derive estimates for the cosmological bulk flow from the SFI++ Tully-Fisher (TF) catalog. For a sphere of radius centered on the MW, we derive a bulk flow of towards Galactic within a error. Within a we get towards within a error. These directions are at a with the Supergalactic plane, close to the apex of the motion of the Local Group of galaxies after the Virgocentric infall correction. Our findings are consistent with the CDM model with the latest WMAP best fit cosmological parameters. But the bulk flow allows independent constraints. For WMAP inferred Hubble parameter and baryonic mean density parameter , the constraint from the bulk flow on the matter density , the normalization…
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