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A Collapsar-disk Origin for GW190814

  • Authors: Vishal Baibhav, Brian D. Metzger, Lam Hui

Vishal Baibhav et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure A1.

Predicted local rate of GW190814-like mergers, RGW190814 = fm RLGRB (Equation (A1) with ϵfragϵLGRB = 1), for fm  =  0.01, 0.05, and 0.10 (top three rows), compared with the measured LVK rate for GW190814 (bottom). The shaded band marks the measured 90% interval (1–23 Gpc−3 yr−1) and the dashed line its median (7 Gpc−3 yr−1; R. Abbott et al. 2020); predicted rates use ﹩{R}_{{\rm{LGRB}}}=7{9}_{-33}^{+57}\,{{\rm{Gpc}}}^{-3}\,{{\rm{yr}}}^{-1}﹩ (G. Ghirlanda & R. Salvaterra 2022). The fm  =  0.05 and fm  =  0.10 cases overlap the measured posterior, while fm  =  0.01 lies at the low-rate edge.

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