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Across the Universe: GW231123 as a Magnified and Diffracted Black Hole Merger

  • Authors: Srashti Goyal, Hector Villarrubia-Rojo, Miguel Zumalacárregui

Srashti Goyal et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure B2.

GW231123 source-frame component masses vs. total macro-magnification μ (embedded PL, NRSur). Lines and shaded bands show the median and 95% intervals as functions of μ, obtained from mass-sheet transformations; the gray region marks the pair-instability mass gap. Contours show the 95% c.l. 2D posteriors of (μm1,2) under the κ = γ (SIS) closure, which gives ﹩\mu =5.{0}_{-3.9}^{+12.0}﹩ (95% c.l.). The dot marks μ ≃ 23, where the median primary mass falls below the gap.

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