Reconstructing the history of structure formation using redshift distortions
Yong-Seon Song, Will J. Percival (Portsmouth, ICG)

TL;DR
This paper discusses how redshift-space distortions in galaxy velocities can be used to probe the history of cosmic structure formation and test dark energy models without requiring detailed bias knowledge.
Contribution
It demonstrates that the parameter combination $f\sigma_8^{\rm mass}$ from redshift distortions effectively tests dark energy and gravity theories, even without bias or $\sigma_8^{\rm mass}$.
Findings
Redshift-space distortions provide a bias-independent test of structure growth.
The $f\sigma_8^{\rm mass}$ parameter constrains dark energy models.
Measuring galaxy bias enables tests of the equivalence principle.
Abstract
Measuring the statistics of galaxy peculiar velocities using redshift-space distortions is an excellent way of probing the history of structure formation. Because galaxies are expected to act as test particles within the flow of matter, this method avoids uncertainties due to an unknown galaxy density bias. We show that the parameter combination measured by redshift-space distortions, provides a good test of dark energy models, even without the knowledge of bias or required to extract from this measurement (here is the logarithmic derivative of the linear growth rate, and is the root-mean-square mass fluctuation in spheres with radius Mpc). We argue that redshift-space distortion measurements will help to determine the physics behind the cosmic acceleration, testing whether it is related to dark energy…
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