Black hole on a chip: how a quantum processor played the role of an information maze ✛

Original: "Simulating Black Hole Thermality and Interior Scrambling on a Superconducting Quantum Processor"
arXiv:2608.19318v1 · 2026-08-19 · CC BY 4.0 · 2 min
On a superconducting processor, the horizon, temperature, and chaos of a black hole were reproduced in a single spin chain.

A black hole is a maze with no way out. But what happens to the information inside? To test this, physicists didn't fly to the nearest hole; instead, they built a tiny replica on a quantum processor. The maze was played by a chain of 32 superconducting qubits, where each step leads only forward, like a one-way corridor.

The event horizon is the boundary beyond which light cannot return. In the model, it was created by changing the transition rules between spins: outside, a signal can go both ways, but inside, only inward.

To understand the geometry of the maze, the scientists launched a single excitation and traced how its energy depends on momentum. Outside, they saw a familiar picture: two branches, like waves on water. At the horizon, one branch flattened — meaning the signal gets stuck. Inside, new points appeared where energy goes to zero, and all paths lead only deeper. For the first time, on a single device, they saw the light cone tilt: beyond the horizon, even light cannot turn around.

The hole's temperature was measured without a thermometer: they placed an excitation just beyond the horizon and watched when it reached an external node. The hotter the hole, the faster the signal arrives. This trick is like gauging an oven's heat by how quickly bread browns.

But the maze doesn't just bend paths: it also scrambles everything that falls in. To see this, they turned on interactions between spins. In the free model, information spread slowly, like ink in cold water. With strong interactions, it began to spread exponentially, as if each step in the maze randomly rearranged the walls. This is quantum chaos: a measure of how quickly a black hole forgets what fell in.

Previously, geometry and chaos were studied separately, in different systems. Here, they were combined in a single experiment, showing that a quantum processor can serve as a testbed for the most pressing questions about black holes. The next step is to test how information returns from the maze if the hole evaporates. Perhaps the answer is already close.

To extract the dispersion on 24 qubits, 4099 two-qubit CZ gates were needed after translation — a record depth for such simulations on superconducting hardware. In scrambling experiments, the number of CZ gates reached 5028 for intermediate values of φ.

The idea of simulating a black hole on a quantum computer echoes Greg Egan's novel 'Schild's Ladder', where physicists create artificial universes with tunable laws. Here, not the entire universe is tuned, but only a tiny part, the horizon and interior of a black hole.

\omega(k) = v \sin(2k) \pm 2u \cos(k)
Excitation energy as a function of momentum; the plus/minus sign corresponds to two branches, the slope is determined by the parameter v.
T_H = \frac{1}{4\pi} \left. \frac{d f(x)}{dx} \right|_{x=x_h}
Temperature is proportional to surface gravity; for the chosen profile f(x) = (π/2) tanh(α(x-x_h)) one obtains T_H = α/8.
T_H^{(est)} = \frac{\gamma}{t_p}
Temperature estimate from the inverse peak time of the density at the outer site; γ is a calibration constant depending on the protocol.
Scientists
Jacob BekensteinStephen HawkingJohn Stewart BellFritz ZwickyKarl SchwarzschildAlain Aspect
Concepts
black hole thermodynamics surface gravity analog black hole Hawking radiation ibm quantum processor cryogenic microwave measurement hawking area law inner horizon Bekenstein-Hawking entropy cryogenic sensing horizon area quantum simulator syk model cooling heat engine scalar perturbations thin film thermal management innermost stable circular orbit quantum simulation quantum black hole thermodynamics