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Implications of Low Neutron Star Merger Rates for Gamma-Ray Bursts, r-process Production, and Galactic Double Neutron Stars

  • Authors: Maya Fishbach, Alexander P. Ji, Wen-fai Fong, Tom Y. Wu, Jillian C. Rastinejad, Aditya Vijaykumar, Hsin-Yu Chen

Maya Fishbach et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 3.

Inferred merger rates for δ-function mass distributions of equal-mass binaries. The posteriors on the merger rates of GW170817-like and GW190425-like mergers are shown as violins (matching their chirp mass to the corresponding component mass of an equal-mass binary). At masses for which there are no detections, we show the 90% upper limit on the inferred rate under a Jeffreys prior. If the BNS mass distribution is skewed to significantly lower masses than we consider (component masses ≲1 M), the merger rate can be at most a factor of ∼2–3 higher than our reported merger rate.

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