Complexity Gets Tangled Midway ✎ express

Original: "Page transition for the complexity of an evaporating black hole"
arXiv:2607.21734 · 2026-07-23 · arXiv non-exclusive · independent analysis · 2 min
The complexity of a quantum system sharply changes its behavior when the system grows beyond half of the whole.

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Water turns to ice at zero degrees — sharply, with no intermediate states. Something similar happens to complexity when we take a random quantum state of an entire system and look only at a part of it. As long as that part occupies less than half the system, its complexity grows smoothly. But as soon as the fraction crosses 50%, a jump occurs.

Here, complexity is a measure of how hard it is to build the desired quantum state from simple building blocks by performing elementary operations.

This transition has been dubbed "Page-like," after the Page curve for information in black holes. The authors go further and explain the cause. Before the midpoint, complexity is dictated by the energy spectrum (the set of available levels), and after, by the specific choice of basis: that is, how we describe the states. In a small town, order might be set by general laws, but in a large one, you also have to account for who lives in each house.

Then the idea was applied to an evaporating black hole in anti-de Sitter space coupled to a thermal bath. Using a toy model, a quantum circuit with random evolution, physicists showed that the complexity of the radiation also undergoes a sharp transition. In the holographic description, this transition is linked to the emergence of an "island": a region inside the black hole that suddenly starts contributing to the volume.

The volume of this island, computed via the holographic recipe "complexity = volume," is exactly what explains the jump.

This resolves the apparent paradox: the complexity of the radiation is not lost but rearranged as the black hole ages. And again, half turns out to be the threshold, just like water at zero degrees.

The complexity transition at half the system is a direct relative of the "Page transition" for entanglement entropy, which shows that information about a black hole starts leaking out exactly at the midpoint of its life.

Scientists
Ludwig BoltzmannRudolf ClausiusErwin SchrödingerHugh Everett IIIStephen HawkingJacob Bekenstein
Concepts
black hole evaporation information loss black hole information paradox phase transition analogy quantum corrections evaporation topological transition holographic dark energy remnant gap barrow entropy complexity Hawking radiation holographic principle Penrose process event horizon hawking radiation anomalies black hole accretion exotic phase transitions quantum classical transition