The Hidden Spin of Black Holes ✎ express

Original: "Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0"
arXiv:2606.12205 · 2026-06-10 · arXiv non-exclusive · independent analysis · 2 min
The spin of merging black holes points to their birthplaces — quiet galactic disks or bustling star clusters.

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Two black holes spiraling toward each other resemble figure skaters in a pair spin: each rotates about its own axis, and together they weave a shared dance. This collective twist, the so-called effective spin, can be measured by astronomers from the gravitational waves rippling outward from the pair, like ripples on a pond. In the new study, scientists analyzed the latest catalog of such events, compiled by the LIGO, Virgo, and KAGRA detectors.

It turns out that most pairs spin very weakly: their effective spin clusters near zero, as if the skaters barely rotate. But some pairs show a noticeably stronger twist, and it more often points in the same direction as their orbital motion. Previously, researchers thought the distribution of these twists was simply skewed to one side, but the new analysis reveals a central "cloud" of weakly spinning pairs, with distinct "outliers" beyond it that have strong spins.

Effective spin is not just the sum of two rotations. If the black holes' axes are tilted relative to each other, their contributions can partially cancel out, like two tops launched at an angle.

Particularly intriguing is that among the most massive pairs (from 47 to 65 solar masses), those with a twist opposite to the orbital motion are slightly more common. However, this asymmetry is not very confident: the odds in its favor are about 13 to 1, and if one suspicious event with data glitches is removed, only 5 to 1. Nevertheless, such an excess of "negative" spins could point to a special birth pathway: black holes that themselves formed from previous mergers of other black holes, and then merged again. Such "hierarchical" mergers are thought to occur more often in dense gas disks around supermassive black holes at the centers of galaxies.

A solar mass is about 333,000 Earth masses. So a black hole of 47 solar masses weighs as much as 15 million of our planets.

In other words, by measuring the hidden twist of colliding black holes, astronomers can peer into the corners of the Universe where these pairs were born. A weak twist likely indicates quiet stellar outskirts; a strong, unidirectional twist points to turbulent gas disks in galactic cores. Each new merger adds a stroke to the map of cosmic "maternity wards."

The effective spin of a black hole pair can range from –1 to +1. Zero means that the spin axes are either nearly not tilted or their contributions cancel each other out.

In Carl Sagan's novel "Contact," an alien signal contains blueprints for a machine that uses rotating black holes to travel through spacetime.

\chi_\mathrm{eff} = \frac{m_1 \chi_1 \cos\theta_1 + m_2 \chi_2 \cos\theta_2}{m_1 + m_2}
The effective spin ($\chi_\mathrm{eff}$) depends on the masses ($m_1$, $m_2$), the individual spins ($\chi_1$, $\chi_2$), and the tilt angles ($\theta_1$, $\theta_2$) of the black holes' spin axes relative to the orbital angular momentum.
Scientists
John Archibald WheelerJacob BekensteinFritz ZwickyKarl SchwarzschildStephen HawkingSubrahmanyan Chandrasekhar
Concepts
effective spin chi squared distribution gravitational wave echoes gw190814 gwtc eccentric black hole binary gravitational wave eccentricity galaxy distribution gravitational wave echo