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Accretion of Primordial Black Holes in Stellar Interiors

  • Authors: Matteo Cantiello, Ore Gottlieb, Cameron Norton, Matthew Kleban, Ken Van Tilburg

Matteo Cantiello et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 3.

Opacity (top) and cumulative optical depth (bottom) as a function of r/rS for MBH = 10−16, 10−13, and 10−11 M⊙. Thick translucent lines show the total opacity; dashed lines show Klein–Nishina-corrected scattering; and dotted lines show Kramers free–free absorption. The vertical dotted line marks the θe = 1 boundary separating the Klein–Nishina-suppressed and Thomson regimes. The horizontal dashed line in the lower panel marks τ = 1.

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