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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 A4.

Sensitivity of wave-optics diffraction to the external potential. Each panel shows the caustics associated to the microlens, the time-domain amplification I(τ), and the corresponding frequency-domain amplification factor ∣F(f)∣, considering the total and diffractive contributions (labeled “WO”). Top panels: varying the external potential strength, assuming κ = γ, at fixed microlens position. Bottom panels: varying the microlens position angle at fixed external potential. Although macroscopic magnification is achromatic in geometric optics, the external potential modifies the microlensing caustics and time-delay response, producing frequency-dependent distortions in F(f).

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