Self-interacting scalar field dark matter produces non-universal core-halo scaling relations that depend on interaction strength, sign, and halo evolutionary stage, extending beyond standard fuzzy dark matter.
MNRAS000, 1–13 (2025)
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Core-halo scaling relations in self-interacting scalar field dark matter
Self-interacting scalar field dark matter produces non-universal core-halo scaling relations that depend on interaction strength, sign, and halo evolutionary stage, extending beyond standard fuzzy dark matter.