A White Hole in the Lens: What the Telescope Will See express

Original: "Using horizon shadows to distinguish a black hole and a white hole"
· Chengyu Bi, Zhoujian Cao
arXiv:2607.20945 · 2026-07-23 · CC BY 4.0 · 1 min
Calculations show what a rotating white hole looks like and how its image differs from a black hole's.

A black hole is a place from which nothing can escape. But some theories allow that deep inside, at the quantum level, it might bounce and turn into its opposite — a white hole, which only spews out matter and light.

A group of physicists built a computer model of such a transformation. They took a rotating black hole and traced the paths of light rays from the hot disk around it — first while the hole is still black, and then after it has become white. For the black hole, the familiar picture emerged: a bright crescent and a dark void in the center. But when light from the previous universe passed through the white hole, the image became completely different.

A white hole does not absorb light but emits it outward. So it has no shadow — instead, light gathers into intricate rings.

Because of the hole's rotation, spacetime twists, and light rays bend in strange ways. The synthetic image showed asymmetric, nested rings of varying brightness. The faster the rotation and the stronger the tilt, the more complex the pattern. The authors also calculated how this light would be polarized. It turned out that from ring to ring, the direction of polarization changes sharply, in a jump — something not seen in black holes.

This "ragged" polarization is the key to identifying a white hole. If future networks of telescopes, working as a single giant eye (the method of interferometry), spot such a pattern, it would be strong evidence for a quantum bounce.

The rotation of a white hole twists space itself — an effect known as "frame-dragging." Because of it, the light rings in the image become asymmetric, as if stretched to one side.

In Stanislaw Lem's novel "Fiasco," an alien civilization uses a white hole as a weapon capable of destroying entire planetary systems.

Scientists
Stephen HawkingJacob BekensteinJohn Archibald WheelerFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
black hole accretion black hole light bending accretion disk wind ringdown apparent horizon hawking radiation mechanism iron k alpha reverberation x ray binary iron line inner horizon hawking radiation anomalies kerr metric reverberation mapping debris disk Bekenstein-Hawking entropy wave amplification photon sphere broad emission lines gap Penrose process