Laboratory Black Holes: Playing with Temperature express

Original: "On the dilaton gravity of analogue black holes"
arXiv:2605.11046 · 2026-05-11 · CC BY 4.0 · 1 min
In superconducting circuits, physicists recreated black holes and learned to manipulate their thermal properties, impossible for real ones.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

An ordinary kettle: you heat it up — temperature rises, molecular chaos grows, and steam shoots out. But in the lab, they've created a peculiar "kettle"—an analog black hole made from superconducting circuits cooled to the extreme. The idea of William Unruh allowed them to mimic the key traits of real black holes: trapping waves and the temperature predicted by Hawking.

The main oddity: here, the link between heating and entropy (a measure of disorder) can be severed. In a real black hole, temperature is rigidly tied to mass — the heavier it is, the colder it gets. But in the lab version, you can change it without touching the internal state: as if the kettle heats up, but no steam comes out. The system's behavior splits into two independent halves — thermal and "disorderly."

A black hole with the mass of the Moon has a temperature of about 1.7 degrees above absolute zero.

Yet a surprise: no known model of gravity describes these samples. The scientists took an inverse approach — instead of tweaking theory, they engineered superconducting circuits with desired properties. Thus, the quest for quantum rules for curved spacetime turns into a precise engineering task.

It was Jacob Bekenstein who first suggested that black holes have entropy, linking it to the area of the event horizon.

In the movie "Interstellar," a black hole bends time — analog systems let us see similar effects at the scale of a microchip.

Scientists
Stephen HawkingJacob BekensteinWilliam UnruhFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
analogue black holes quantum gravity analogues black hole thermodynamics surface gravity gravitational instanton white hole liquid helium temperature tidal charge dilaton Hawking radiation remnant quantum corrections syk model hawking area law analog black hole quantum bounce alternative gravity theories hawking radiation anomalies wald entropy