Peculiar-velocity distribution functions and 21-cm fluctuations

TL;DR

This paper refines predictions of 21-cm background fluctuations by accurately calculating the joint probability distribution of peculiar velocities, revealing small but sometimes significant errors in previous models.

Contribution

It provides a full calculation of the joint PDF of peculiar velocities at two points, improving the accuracy of 21-cm fluctuation predictions.

Findings

Errors from previous approximations are generally small, less than a few percent.

The full joint PDF calculation slightly increases computational time by a few percent.

Correct modeling of velocity correlations can be important at specific scales and redshifts.

Abstract

Predictions for observables involving the cosmological 21-cm background require calculations of spatial correlations of star formation rate densities (SFRDs) which have a nonlinear dependence on the baryon-dark matter relative velocity. Prior work derived these SFRD correlations with a simplifying assumption that neglected the difference between the correlations of the components of the velocity parallel and perpendicular to the separation between the two points being correlated. Here we calculate the full joint PDF of the squares of the peculiar velocity at two different points. The error that arises in predictions for 21-cm fluctuations if this subtlety is overlooked is generally less than a few percent, but it can be larger for some values of wavenumber $k$ and redshift $z$ if there are cancellations between different contributions to the total signal. The correct expression is easily implemented and increases the run time of the code by only a few percent.