Black Holes: Light's Hidden States ✎ express

Original: "Black Hole Thermodynamics via Tsallis Statistical Mechanics and Phase Transitions Probed by Optical Characteristics"
arXiv:2605.02429 · 2026-05-04 · arXiv non-exclusive · independent analysis · 1 min
The light ring around a black hole reveals its temperature, pressure, and ability to 'freeze' or 'boil'.

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Black holes aren't faceless devourers. Sometimes they behave like water: they can 'freeze' or 'boil', changing their internal state. Scientists described this by modeling light near a black hole as a gas. This gave rise to a generalized formula for entropy (a measure of disorder), building on the ideas of Bekenstein and Hawking. The twist: this disorder is proportional to the hole's area, not its volume — the exact opposite of what we see in a cup of coffee or a cloud of steam.

Like water with its ice, liquid, and vapor, black holes abruptly switch between distinct states.

The key is the light ring, formed by spacetime curvature. Its properties — rotation speed, beam divergence — sensitively mirror the temperature and pressure of the black hole. By watching the ring, you can literally see the hole undergoing its transformations.

Light trapped by gravity tells the full story of a black hole's hidden life — no mysticism, just plain physics.

A black hole's entropy — its measure of disorder — grows with surface area, not volume. It's as if a room seemed messier because of the size of its walls, not what's inside.

The famous glowing ring from 'Interstellar' is exactly the light ring that gives away a black hole's secrets.

Scientists
Jacob BekensteinStephen HawkingFritz ZwickyKarl SchwarzschildSubrahmanyan ChandrasekharRainer Weiss
Concepts
black hole thermodynamics Bekenstein-Hawking entropy wald entropy hawking area law Hawking area theorem reissner nordstrom black hole logarithmic correction schwarzschild metric no-hair theorem surface gravity enthalpy Stefan–Boltzmann law entropic shadow critical collapse mass inflation charge to mass ratio event horizon stability kerr metric holographic dark energy topological transition