Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores
Carlos Tena-Contreras, Ivan Alvarez-Rios, Francisco S. Guzman, Jens Niemeyer

TL;DR
This study uses 3D simulations to analyze how self-interaction and ideal gas presence affect binary mergers of bosonic dark matter cores, revealing interaction-dependent outcomes and core stability.
Contribution
It demonstrates how self-interaction and gas influence the mass and stability of merger remnants in bosonic dark matter models, providing new insights into core formation.
Findings
Repulsive self-interaction increases final core mass.
Attractive interaction enhances mass loss during mergers.
Stable solitonic cores form even with gas dominance.
Abstract
We study binary mergers of dark matter cores in the Bose-Einstein condensate (BECDM) model. We include two scenarios: scalar self-interaction and the presence of a gravitationally coupled ideal gas. Using 3D simulations of the Gross-Pitaevskii-Poisson and Schr\"odinger-Poisson-Euler systems, we analyze the properties of the resulting remnants. We find that the final core-mass ratio reaches a stable average value after the merger. Repulsive self-interaction increases the mass of the final solitonic core, while attractive interaction enhances mass loss. In mergers involving an ideal gas, namely of fermion-boson stars, a stable solitonic core always forms in the bosonic component, even when the gas dominates, whereas the gas itself does not form a compact core. We explain these results using energy scalings and find that without self-interaction, equilibrium cores follow ,…
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