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Probing the Nature of Dark Matter Self-interactions through Observations of Massive Black Hole Mergers

  • Authors: Zachary J. Hoelscher, Kelly Holley-Bockelmann, Akaxia Cruz, N. Nicole Sanchez

Zachary J. Hoelscher et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 5.

Average p-values (black dots) for comparing cosmic times (left) or mass ratios (right) of mergers with CDM to mergers with SIDM-1. We indicate the 95th percentile with an X. The red line indicates the significance threshold of 0.05. For differentiating between CDM and SIDM-1, we wish to have the 95th percentile below the significance threshold. We find that ∼70 mergers are sufficient to attain this when comparing cosmic times, or ∼160 mergers when comparing mass ratios.

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