Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
Matteo Nori, Marco Baldi

TL;DR
This paper investigates how the properties and scaling relations of Fuzzy Dark Matter haloes are affected by their cosmological environment, using N-body simulations to analyze individual systems' evolution, morphology, and merger history.
Contribution
It introduces the first detailed study of FDM halo scaling relations in a cosmological setting, highlighting the influence of dynamical state and environment.
Findings
Scaling relations are modified in realistic cosmological environments.
Relations hold mainly for relaxed, spherical systems.
AX-GADGET accurately reproduces FDM solitonic cores.
Abstract
Dark matter models involving a very light bosonic particle, generally known as Fuzzy Dark Matter (FDM), have been recently attracting great interest in the cosmology community, as their wave-like phenomenology would simultaneously explain the longstanding mis-detection of a dark matter particle and help easing the small-scale issues related to the standard Cold Dark Matter (CDM) scenario. With the present work, we initiate a series of papers aiming at investigating the evolution of FDM structures in a cosmological framework performed with our N-body code AX-GADGET, detailing for the first time in the literature how the actual scaling relations between solitonic cores and host haloes properties are significantly affected by the dynamical state, morphology and merger history of the individual systems. In particular, in this first paper we confirm the ability of AX-GADGET to correctly…
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