Simple

Toy Black Hole and the New Rules of Gravity ⚡ экспресс

Original: "Stationary BTZ space-time in Ricci-Inverse and $$f(\mathcal{R})$$ gravity theories"
arXiv:2410.11922 · 2024-10-15 · CC BY 4.0 · ⏱ 1 min · General Relativity HEP Theory
A simple model of a black hole in a two-dimensional world helps test a modified theory of gravity.
Abstract

Researchers explored a peculiar black hole (BTZ) in a fresh theory of gravity. Turns out, this beast exists, but the cosmic push-back force shifts. They also tracked particle paths around it—they deviate from what Einstein would say. What other black hole mysteries might tweaked gravity unlock?

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Spacetime in Einstein's theory behaves like a rubber sheet: massive bodies bend it. But the accelerated expansion of the Universe hints that the sheet may have unusual properties. To test new rules of gravity, physicists use simplified models — for example, black holes in two-dimensional worlds. One such "toy" is the BTZ black hole: it lives on a plane but keeps the main features of the real thing.

In a modified theory of gravity, such a hole also appears, but the parameter controlling the galaxies flying apart becomes different. Particles and light move along new trajectories that were calculated precisely — like a ball rolling on a curved sheet. Comparison with the Einstein case revealed subtle differences. Perhaps one day they will make it possible to do without hypothetical dark energy to explain the acceleration of the cosmos.

🎯 In a two-dimensional universe, a black hole is not a sphere but a circle, and its event horizon is a simple line. Yet the formulas for an infalling observer are almost the same as in the three-dimensional case.

🎬 Physicists often construct worlds with fewer dimensions — like in Edwin Abbott's novel "Flatland", where flat beings are unaware of height. The BTZ black hole is their version of a black hole.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesStephen HawkingJacob Bekenstein
Tags
black hole dark energy spacetime curvature
Laws
Friedmann equationsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsequivalence principle
Original: arXiv:2410.11922 · CC BY 4.0 · bridge42worlds