The diversity of core–halo structure in the fuzzy dark matter model. Issue 1 (12th January 2022)

• Record Type: Journal Article
• Authors: Chan, Hei Yin Jowett; Ferreira, Elisa G M; May, Simon; Hayashi, Kohei; Chiba, Masashi
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 511:Issue 1(2022)
• Page Start: 943
• Page End: 952
• Publication Date: 2022-01-12
• Subjects: methods: numerical -- software: simulations -- galaxies: haloes -- dark matter -- cosmology: theory; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac063
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: In the fuzzy dark matter (FDM) model, gravitationally collapsed objects always consist of a solitonic core located within a virialized halo. Although various numerical simulations have confirmed that the collapsed structure can be described by a cored Navarro–Frenk–White-like density profile, there is still disagreement about the relation between the core mass and the halo mass. To fully understand this relation, we have assembled a large sample of cored haloes based on both idealized soliton mergers and cosmological simulations with various box sizes. We find that there exists a sizeable dispersion in the core–halo mass relation that increases with halo mass, indicating that the FDM model allows cores and haloes to coexist in diverse configurations. We provide a new empirical equation for a core–halo mass relation with uncertainties that can encompass all previously found relations in the dispersion, and emphasize that any observational constraints on the particle mass m using a tight one-to-one core–halo mass relation should suffer from an additional uncertainty of the order of 50 per cent for halo masses ${\gtrsim} 10^9 \, [8\times 10^{-23} \, \mathrm{eV}/(mc^2)]^{3/2} \, \mathrm{M}_\odot$ . We suggest that tidal stripping may be one of the effects contributing to the scatter in the relation.