The diversity of core-halo structure in the fuzzy dark matter model

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 greater than or similar to 10(9) [8 x 10(-23) eV/(mc(2))](3/2) M-circle dot. We suggest that tidal stripping may be one of the effects contributing to the scatter in the relation.

Automated summary

In the fuzzy dark matter model, there is a significant dispersion in the core-halo mass relation, increasing with halo mass. A new empirical equation for the core-halo mass relation is provided, with uncertainties encompassing previously found relations. Any observational constraints on particle mass using a tight one-to-one core-halo mass relation should consider an additional uncertainty of about 50%.