Using measurements of the cosmic bulk flow to constrain $f(R)$ Gravity
Jacob Seiler (1,2), David Parkinson ((1) School of Mathematics and, Physics, University of Queensland (2) ARC Centre of Excellence for All-sky, Astrophysics (CAASTRO))

TL;DR
This study uses cosmic bulk flow measurements and simulations to constrain $f(R)$ gravity, finding that the strength of this modified gravity must be limited to match observed bulk flows, thus providing a test for alternative gravity theories.
Contribution
The paper demonstrates how bulk flow measurements can effectively constrain the strength of $f(R)$ gravity, using simulations and observational data to set upper limits on $f_{R0}$.
Findings
Bulk flow measurements are consistent with $ ext{Lambda CDM}$ predictions for $f_{R0} o 10^{-5}$.
Higher $f_{R0}$ values predict larger bulk flows, inconsistent with observations.
Constraints suggest $f_{R0}$ must be less than or equal to $10^{-4}$ to match data.
Abstract
As an alternative explanation for the cosmic acceleration, theories of gravity can predict an almost identical expansion history to standard CDM, yet make very different predictions for the growth of cosmological structures. Measurements of the cosmic bulk flow provides a method for determining the strength of gravity over the history of structure formation. We use the modified gravity N-body code ECOSMOG to simulate dark matter particles and make predictions for the bulk flow magnitude in both CDM and gravity. With the peculiar velocities output by ECOSMOG we determine the bulk flow at depths ranging from Mpc to Mpc, following the redshift and sky distribution of the 2MASS Tully-Fisher survey (2MTF). At each depth, we find that the CDM and simulations produce bulk flow measurements that are consistent with…
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