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Black holes behave like boiling water ⚡ экспресс

Original: "Dunkl-Corrected Deformation of RN-AdS Black Hole Thermodynamics"
· Maryem Jemri
arXiv:2512.19200 · 2025-12-22 · CC BY 4.0 · ⏱ 1 min · HEP Theory
Scientists discovered that black holes can behave like boiling water: they have a critical point and obey familiar laws of thermodynamics.
Abstract

Scientists have come up with a new type of charged black holes by adding unusual derivatives with reflections to Einstein's equations. The thermal properties of such holes resemble the behavior of a fluid: they can undergo phase transitions, just like water turning into steam. Could it be that black holes can 'boil'?

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Scientists applied an unusual mathematical approach in the equations of искривления пространства-времени and obtained a new type of charged чёрных дыр. Their behavior turned out to be surprisingly familiar: this is how вода in a pot behaves when it starts to boil. At a certain combination of pressure, volume, and temperature, the difference between a "liquid" and "gaseous" black hole vanishes. This is exactly like the critical point of water: steam and liquid become indistinguishable.

For all such black holes, the ratio of these three quantities remains constant, like a universal culinary proportion.

Even Стивен Хокинг and Яаков Бекенштейн proved that black holes have temperature and энтропия (a measure of disorder). The new research adds that the transitions between states of these objects obey the same laws as steam boiling. Most unexpectedly: if you remove the mathematical "seasoning" from the calculations, the black hole behaves exactly like an ideal gas describing the transformation of water into steam.

🎯 Black holes are not eternal: due to Hawking radiation, they slowly evaporate. A tiny black hole could "boil" away and vanish in a fraction of a second.

\frac{P_c v_c}{T_c} = \text{const}
P_c — critical pressure, v_c — critical specific volume, T_c — critical temperature; their ratio is constant for all studied black holes.
Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole entropy spacetime curvature Water
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2512.19200 · CC BY 4.0 · bridge42worlds