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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 6.

Here we show the distribution of p-values for comparing cosmic times (left) and comparing mass ratios (right). For cosmic times, this corresponds to ∼70 mergers, whereas for mass ratios, this corresponds to ∼160 mergers. These plots show the fraction of the 10,000 p-values that live in each bin.

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