Note that we use equation B4 withfh =f r/n, while Berentzen et al

hc,n(f) = p N(f)h s,n(f) = 37 √ 5 64 √ 6π2/3 (GM)5/6 c3/2d(z) p g(n, e)f −1/6, (B4) withMbeing the chirp mass of the binary,d(z)the comoving distance from the observer, g(n, e) = n4 32 Jn−2(ne)−2eJ n−1(ne) + 2 n Jn(ne) + 2eJn+1 −J n+2(ne · 1963

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Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies

astro-ph.GA · 2025-12-12 · unverdicted · novelty 6.0

Cosmological zoom-in simulations demonstrate rapid SMBH mergers in dense high-z galaxies within 4-35 Myr after binary binding, matching JWST compact galaxy observations.

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Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies astro-ph.GA · 2025-12-12 · unverdicted · none · ref 3
Cosmological zoom-in simulations demonstrate rapid SMBH mergers in dense high-z galaxies within 4-35 Myr after binary binding, matching JWST compact galaxy observations.

Note that we use equation B4 withfh =f r/n, while Berentzen et al

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