Quantum Computer Played the Role of a Black Hole: What Physicists Saw ✛

Original: "Simulating Black Hole Thermality and Interior Scrambling on a Superconducting Quantum Processor"
arXiv:2608.19318v1 · 2026-08-19 · CC BY 4.0 · 1 min
Scientists built a tiny black hole from qubits and measured its temperature and chaos.

A black hole is a place from which even light cannot escape. To study its behavior, scientists built a tiny replica on a quantum computer. They used a chain of 32 qubits, like a one-way street: the signal can only move forward, toward the center of the hole.

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

First, the physicists launched a single signal and observed how its energy depends on velocity. Outside, everything is normal: the signal can move in both directions. At the boundary, one of the energy branches became flat — meaning the signal gets stuck. Inside, new features appeared, and all paths lead only deeper. This is how they saw the light cone tilt: beyond the horizon, even light cannot turn around.

To measure the hole's temperature, they placed the signal just beyond the boundary and timed how long it took to reach the outer qubit. The hotter the hole, the faster the signal arrives. This is like judging the heat of an oven by how quickly bread toasts. When they turned on interactions between qubits, information scrambled very quickly, as if walls in a maze were being rearranged at every step. Previously, such phenomena were studied separately, but now they have been combined in a single experiment.

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