Polarized Light Reveals Black Hole Spin ✛ ✎ ✦

Original: "Signatures of Black Hole Spin in Horizon-Scale Polarimetry"
arXiv:2607.14218 · 2026-07-15 · arXiv non-exclusive · independent analysis · 1 min
Polarized light around black holes works like a compass needle, pointing to their spin and magnetic vortices.

Black holes aren’t frozen: they spin rapidly, dragging space itself along, as predicted by Einstein’s theory. The first model of a non-rotating hole was built by Karl Schwarzschild, but reality is more dynamic. Infalling gas forms a scorching disk, where plasma accelerates to near light speed and emits radio waves. As light travels through the magnetized medium, it becomes polarized: its waves oscillate in a single plane, like compass needles following the field lines.

By linking radio telescopes into a virtual antenna the size of Earth, astronomers captured this radiation from two supermassive giants — M87* and Sagittarius A*. Comparison with computer simulations revealed that magnetic fields near the hole’s edge are twisted into spirals, and it is these that launch plasma jets flying thousands of light-years, like projectiles from a magnetic sling.

But the biggest surprise: a rotating hole can transfer its spin energy through these fields — a mechanism discovered by Penrose. Thus the abyss turns into an engine powering the jets. The hole’s mass bends the light itself (gravitational lensing), while frame-dragging adds further distortions. Understanding these effects refines spin measurements and the shape of gravitational waves from black hole mergers.

The black hole at the center of the Milky Way, Sagittarius A*, changes its polarization every few minutes, while M87* takes a few days. The reason is mass: the lighter the hole, the faster its processes.

In the movie Interstellar, the rotating black hole Gargantua was visualized taking into account light bending and frame-dragging — exactly the effects that polarization imaging helps us study.

a_* = \frac{Jc}{GM^2}
Dimensionless spin parameter: J — angular momentum, M — mass, c — speed of light, G — gravitational constant; can take values from –1 to 1.
P = Q + iU = \sum_{m} \beta_m e^{im\phi}
Decomposition of complex linear polarization into azimuthal harmonics: φ — azimuthal angle, coefficients β_m encode magnetic field structure and spin effects.
Scientists
John Archibald WheelerJacob BekensteinStephen HawkingFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
black hole spin spin parameter black hole photon ring photon sphere event horizon horizon area scalar particle iron line astrophysical polarimetry hawking radiation anomalies scalar perturbations Bekenstein-Hawking entropy stellar rotation Hawking radiation mass inflation accretion disk wind spiral arms surface gravity optical vortex spiral