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The effect of thermal velocities on structure formation in N-body simulations of warm dark matter

Leo, M.; Baugh, C.M.; Li, B.; Pascoli, S.

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Authors

M. Leo



Abstract

We investigate the impact of thermal velocities in N-body simulations of structure formation in warm dark matter models. Adopting the commonly used approach of adding thermal velocities, randomly selected from a Fermi-Dirac distribution, to the gravitationally-induced velocities of the simulation particles, we compare the matter and velocity power spectra measured from CDM and WDM simulations, in the latter case with and without thermal velocities. This prescription for adding thermal velocities introduces numerical noise into the initial conditions, which influences structure formation. At early times, the noise affects dramatically the power spectra measured from simulations with thermal velocities, with deviations of the order of ~ Script O(10) (in the matter power spectra) and of the order of ~ Script O(102) (in the velocity power spectra) compared to those extracted from simulations without thermal velocities. At late times, these effects are less pronounced with deviations of less than a few percent. Increasing the resolution of the N-body simulation shifts these discrepancies to higher wavenumbers. We also find that spurious haloes start to appear in simulations which include thermal velocities at a mass that is ~3 times larger than in simulations without thermal velocities

Journal Article Type Article
Acceptance Date Oct 23, 2017
Online Publication Date Nov 13, 2017
Publication Date Nov 13, 2017
Deposit Date Jan 15, 2018
Publicly Available Date Nov 13, 2018
Journal Journal of Cosmology and Astroparticle Physics
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2017
Issue 11
Article Number 017
DOI https://doi.org/10.1088/1475-7516/2017/11/017
Public URL https://durham-repository.worktribe.com/output/1368412
Related Public URLs https://arxiv.org/abs/1706.07837

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