Peculiar Velocities into the Next Generation: Cosmological Parameters From Large Surveys without Bias from Nonlinear Structure
Alexandra Abate (1), Sarah Bridle (1), Luis F. A. Teodoro (2), Michael, S. Warren (3), and Martin Hendry (2) ((1) UCL, (2) University of Glasgow, (3), LANL)

TL;DR
This paper presents a method to accurately estimate the cosmological parameter sigma_8 from peculiar velocity surveys by averaging velocities in grid cells, effectively reducing nonlinear bias and maintaining precision.
Contribution
It introduces a practical averaging technique in grid cells to mitigate nonlinear effects in velocity data, comparable to principal component methods, for unbiased cosmological parameter estimation.
Findings
Averaging velocities reduces nonlinear bias without increasing errors significantly.
The method achieves less than 3% bias in sigma_8 estimation from surveys like 6dFGSv.
Estimated error on sigma_8 is approximately 16% after marginalizing over other parameters.
Abstract
We investigate methods to best estimate the normalisation of the mass density fluctuation power spectrum (sigma_8) using peculiar velocity data from a survey like the Six degree Field Galaxy Velocity Survey (6dFGSv). We focus on two potential problems (i) biases from nonlinear growth of structure and (ii) the large number of velocities in the survey. Simulations of LambdaCDM-like models are used to test the methods. We calculate the likelihood from a full covariance matrix of velocities averaged in grid cells. This simultaneously reduces the number of data points and smooths out nonlinearities which tend to dominate on small scales. We show how the averaging can be taken into account in the predictions in a practical way, and show the effect of the choice of cell size. We find that a cell size can be chosen that significantly reduces the nonlinearities without significantly increasing…
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