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When a Black Hole Can Split Apart ⚡ экспресс

Original: "When Black Holes Can Wear Pants"
arXiv:2606.24642 · 2026-06-23 · CC BY-SA 4.0 · ⏱ 1 min · General Relativity HEP Phenomenology
Black hole splitting is a rare event, possible only with extreme rotation or in other dimensions.
Abstract

Black holes are regions of space with gravity so strong that not even light can escape. Normally, a black hole cannot simply split into two on its own, just like you can't effortlessly tear a soap bubble—a special law that prevents the area from decreasing stops it. Scientists have found that under unusual conditions (such as extremely fast rotation or in spaces with extra dimensions) fragmentation might become possible.

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A black hole is like a spinning drop of viscous liquid. Normally, such a drop tends to stay whole: splitting would reduce its surface area, which contradicts the law of non-decrease of entropy (a measure of disorder, like a broken cup doesn't glue itself back together). For non-rotating black holes, discovered by Karl Schwarzschild, splitting is impossible. However, with furious rotation, centrifugal forces stretch the black hole, and a microscopic fragment can pinch off. This process resembles nuclear fission in the liquid-drop model. Physicists have also considered worlds with extra dimensions, where spacetime curvature behaves differently, and black holes can become unstable, like long liquid threads ready to snap into pieces. Such decay could alter the population of primordial black holes, born in the young Universe.

The connection between the area of a black hole and entropy was established by Jacob Bekenstein and Stephen Hawking. This turned black holes into full-fledged thermodynamic systems.

🎯 Merging black holes, on the contrary, always increases the total area—this process resembles the merging of mercury droplets and is accompanied by powerful [tag:gravitational_waves]gravitational waves[/tag].

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole entropy spacetime curvature gravitational waves
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2606.24642 · CC BY-SA 4.0 · bridge42worlds