How Brane Tension Changes Black Holes express

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
In a multidimensional universe, gravity weakens, stripping light black holes of their horizon.

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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
Fritz ZwickyBernhard RiemannJoseph WeberKarl SchwarzschildKip ThorneRainer Weiss
Concepts
brane world black holes schwarzschild black hole schwarzschild metric brane world gravity wald entropy inner horizon horizon area Hawking area theorem Bekenstein-Hawking entropy innermost stable circular orbit general relativity classical gravity tidal charge logarithmic correction white hole Hawking radiation Birkhoff's theorem photon sphere Lense–Thirring effect entropic shadow