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In the RAR case, when the central fermions are in a state of low degeneracy (θ0 ≪ − 1), we recover the resulting DM spike of ρ ∝ r−3/2 typical of cored halos as the NSIS (see Fig

The typically assumed power-law DM spikes occur only in the case of initial DM configurations in the Boltzmannian regime

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Fermionic Dark Matter spikes: origin and growth of Black Hole seeds

astro-ph.GA · 2024-12-23 · conditional · novelty 6.0

Fermionic dark matter halos around supermassive black holes can form non-power-law spikes or even density depletions, depending on the fermion mass and degeneracy, instead of the universal r^-3/2 spike of power-law halos.

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  • Fermionic Dark Matter spikes: origin and growth of Black Hole seeds astro-ph.GA · 2024-12-23 · conditional · none · ref 4

    Fermionic dark matter halos around supermassive black holes can form non-power-law spikes or even density depletions, depending on the fermion mass and degeneracy, instead of the universal r^-3/2 spike of power-law halos.