Toy Black Hole and the New Rules of Gravity ✛

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
A simple model of a black hole in a two-dimensional world helps test a modified theory of gravity.

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.

\Lambda_m = \Lambda - 6\alpha_1 \Lambda^2 - 108\alpha_2 \Lambda^3 + \frac{5\beta_1}{4\Lambda} + \frac{15\beta_2}{8\Lambda^2} + \frac{7\gamma}{8\Lambda^2}
The cosmological constant receives corrections from all coupling constants
\Lambda_m = \Lambda - 6\alpha_1 \Lambda^2 - 108\alpha_2 \Lambda^3
The corrections depend only on the coefficients of R^2 and R^3
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
fr gravity fq gravity gravitational theory einstein quantum field theory in curved spacetime Lorentz transformations anti de sitter space geodesic equation metric spacetime AdS/CFT correspondence spacetime curvature equivalence principle Wheeler-DeWitt equation Einstein field equations general relativity causal set theory