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The Binary Black Hole Merger Rate Deviates from the Cosmic Star Formation Rate: A Tug of War between Metallicity and Delay Times

  • Authors: Adam P. Boesky, Floor S. Broekgaarden, Edo Berger

Adam P. Boesky et al 2024 The Astrophysical Journal 976 .

  • Provider: AAS Journals

Caption: Figure 7.

BBH merger rate as a function of redshift compared to toy model merger rates assuming a scaled SFRD (left), a scaled SFRD with constant delay times (middle), and a scaled SFRD with a t −1 delay time distribution (right). All simulations are normalized to the same intrinsic merger rate R merge,0. We assumed minimum delay times for the middle and right panel of 20 Myr. Labels and colors are the same as in Figure 1.

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