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Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots

  • Authors: Tak-Pong Woo

Tak-Pong Woo 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 1.

Constraints on boson mass (m22) from combining the soliton size scaling (Equation (1)) with an opacity (column) requirement. The vertical axis shows a characteristic physical scale; we compare the observed effective radius range of LRDs (green band, re ∼ 30–100 pc) with the soliton core radius predicted for Ms = 108–109 M (blue band; dashed boundaries follow ﹩{r}_{c}\propto {m}_{22}^{-2}﹩). The red region marks parameters for which even a maximally loaded core (fg ≈ 1) confined within re rc with ξ ≈ 1 cannot reach NH ≈ 1024 cm−2,. The opacity boundary is evaluated for a representative Ms ∼ 109 M (typical of LRD hosts). The orange shaded area illustrates sensitivity to baryon loading uncertainties by adopting conservative values (fg = 0.1, ξ = 3). The viable region is the overlap between the observed size band and the nontransparent (Compton-thick-capable) region; the region outside the red shaded area corresponds entirely to the nontransparent (Compton-thick capable) regime. The “viable region” is specifically the parallelogram defined by the overlap between the observed size band and this nontransparent regime. Under the direct-mapping assumption (re ∼ rc), this favors m22 ∼ few, and we adopt m22 = 2 as a fiducial baseline for subsequent figures.

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