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Are there any extragalactic high speed dark matter particles in the Solar neighborhood?

Santos-Santos, Isabel; Bozorgnia, Nassim; Fattahi, Azadeh; Navarro, Julio F.

Are there any extragalactic high speed dark matter particles in the Solar neighborhood? Thumbnail


Authors

Isabel Santos-Santos

Nassim Bozorgnia

Julio F. Navarro



Abstract

We use the APOSTLE suite of cosmological hydrodynamical simulations of the Local Group to examine the high speed tail of the local dark matter velocity distribution in simulated Milky Way analogues. The velocity distribution in the Solar neighborhood is well approximated by a generalized Maxwellian distribution sharply truncated at a well-defined maximum “escape” speed. The truncated generalized Maxwellian distribution accurately models the local dark matter velocity distribution of all our Milky Way analogues, with no evidence for any separate extragalactic high-speed components. The local maximum speed is well approximated by the terminal velocity expected for particles able to reach the Solar neighborhood in a Hubble time from the farthest confines of the Local Group. This timing constraint means that the local dark matter velocity distribution is unlikely to contain any high-speed particles contributed by the Virgo Supercluster “envelope”, as argued in recent work. Particles in the Solar neighborhood with speeds close to the local maximum speed can reach well outside the virial radius of the Galaxy, and, in that sense, belong to the Local Group envelope posited in earlier work. The local manifestation of such envelope is thus not a distinct high-speed component, but rather simply the high-speed tail of the truncated Maxwellian distribution.

Citation

Santos-Santos, I., Bozorgnia, N., Fattahi, A., & Navarro, J. F. (2024). Are there any extragalactic high speed dark matter particles in the Solar neighborhood?. Journal of Cosmology and Astroparticle Physics, 2024(03), Article 046. https://doi.org/10.1088/1475-7516/2024/03/046

Journal Article Type Article
Acceptance Date Feb 2, 2024
Online Publication Date Mar 21, 2024
Publication Date Mar 1, 2024
Deposit Date May 20, 2024
Publicly Available Date May 20, 2024
Journal Journal of Cosmology and Astroparticle Physics
Electronic ISSN 1475-7516
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2024
Issue 03
Article Number 046
DOI https://doi.org/10.1088/1475-7516/2024/03/046
Keywords dark matter experiments, hydrodynamical simulations, dark matter simulations, dark matter theory
Public URL https://durham-repository.worktribe.com/output/2346138

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