Image Details

Choose export citation format:

A Unified Dark-matter-driven Relativistic Bondi Route to Black Hole Growth from Stellar to Supermassive Scales

  • Authors: Chian-Shu Chen, Feng-Li Lin

Chian-Shu Chen and Feng-Li Lin 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

Evolution of the QCD PBH mass function for lognormal (top), power-law (middle), and critical-collapse (down) distributions to z = 7 under SIDM–Bondi-aided Eddington accretion with DM mass m = 10−3,−2,−1 eV. The growth triggers early Bondi dominance for m ≳ 10−2 eV to reach 1010M SMBHs. The insets in each figure show the finer structures of the final mass function.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse