Prefab Black Holes: How Remnants of Past Mergers Collide ✛ ✎

Original: "Exploring Hierarchical Merger Scenarios for GW241011 and GW241110"
arXiv:2607.04663v1 · 2026-07-06 · arXiv non-exclusive · independent analysis · 2 min
Astrophysicists have found compelling evidence that black holes can be 'second-generation' — born from the collision of other black holes.

Recently, detectors of gravitational waves recorded two unusual mergers of black holes. Analysis showed that in each pair, one of the black holes wasn't a simple one, but a 'prefabricated' one — it itself formed from the collision of two other holes in the past. It's like playing with a construction set: instead of only picking individual bricks, you sometimes use already assembled blocks.

It's been noticed that offspring black holes spin at almost a constant speed — about 70% of the maximum possible. This peculiarity allows us to recognize them in future observations, like a maker's mark.

The idea of black holes goes back to the calculations of Karl Schwarzschild, and the first attempt to catch gravitational waves was made by Joseph Weber half a century ago. Today we know that galaxies, whose classification was pioneered by Edwin Hubble, often harbor supermassive black holes and gas disks at their centers — ideal places for the birth of 'prefabricated' black holes.

Interestingly, part of the mysterious dark matter could consist of such 'secondary' black holes, left over from the first moments of the Universe. This is still a hypothesis, but such discoveries will help test it.

Gravitational waves carry information through space at the speed of light, and we've learned to read it. To see such mergers also in ordinary light, we'll need spectroscopy — a method that allows us to split light into colors and find lines of hydrogen from heated gas. This will be helped by the Hubble telescope and future observatories. Thus, a new chapter in astronomy will open: unified vision in gravity and light.

Offspring black holes from mergers always spin at roughly the same speed — about 70% of the maximum possible. This makes them easily identifiable in gravitational wave data.

B^i_j = \frac{p(d|H_i)}{p(d|H_j)}
The ratio of the probability of the observed data if hypothesis i is true to the probability if hypothesis j is true. The larger the B, the more the data support hypothesis i.
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
black hole merger binary black hole galaxy merger gw190814 gwtc Generative Adversarial Networks gravitational wave echoes globular cluster event gw170817 common envelope ringdown galactic bulge mass ratio eccentric binary gravitational waves changing agn activity binary star active galactic nucleus gravitational wave catalog black hole binary interaction