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How Brane Tension Changes Black Holes ⚡ экспресс

Original: "Astrophysical environment around a black hole in the braneworld and its optical signatures"
arXiv:2605.26124 · 2026-05-14 · CC BY 4.0 · ⏱ 1 min · HEP Theory General Relativity
In a multidimensional universe, gravity weakens, stripping light black holes of their horizon.
Abstract

Imagine our universe as a stretchy trampoline: a black hole tries to press a dip, but the tension of the fabric (brane energy) prevents it — the horizon doesn't form. And the black hole's shadow and Einstein ring act like the hands of a scale, by which you can 'weigh' the tension of hidden dimensions.

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Our Universe behaves like a stretched elastic sheet: massive bodies dent it, creating spacetime curvature — gravity. In brane-world theory, a hidden dimension is added, and this sheet becomes just a surface in a higher-dimensional space. The brane tension determines how much the sheet dents: the weaker the tension, the weaker the gravity.

Scientists have studied how this affects black holes of the Schwarzschild type, surrounded by a dense cloud of particles. For light holes (less than a star's mass), the weakened gravity might not form a horizon — the boundary from which nothing can escape. Constraints on brane tension come from observations of neutron stars.

An unexpected effect: the black hole's shadow grows while the Einstein ring — the luminous halo around it — shrinks. Measuring these two parameters could reveal the presence of extra dimensions.

Brane theory says we live on a three-dimensional sheet inside a higher-dimensional world, and only gravity can leak into neighboring dimensions.

🎯 If brane tension disappeared, our Universe would become completely flat and devoid of gravity.

🎬 In the film *Interstellar*, highly advanced beings live in five dimensions — much like the brane idea from scientific theories.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole spacetime curvature neutron star
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsFermi–Dirac statisticsequivalence principle
Original: arXiv:2605.26124 · CC BY 4.0 · bridge42worlds