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Gravitational Shooting Gallery: Sighting in on Black Holes

Original: "Black-Hole Scattering in Einstein-scalar-Gauss-Bonnet: Numerical Relativity Meets Analytics"
arXiv:2605.04224v1 · 2026-05-05 · CC BY 4.0 · ⏱ 1 min · General Relativity HEP Theory
A bullseye: simulations of black hole scattering in Einstein-scalar-Gauss-Bonnet theory confirmed analytical predictions with less than a one-degree deviation.
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Black holes can not only swallow matter but also bounce off each other elastically, like billiard balls. Scientists set up a gravitational shooting gallery — and the scattering angle matched the theory to within a degree. In the future, such targeted tests of "hairy" holes will help find cracks in the foundation of general relativity.

🎯 Unlike slow accretion, black hole "hair" here grows almost instantly — within a couple of dynamical timescales. This makes them almost universal objects, carrying a memory of the field from birth.

🎬 In "Interstellar," Gargantua is a portal through time. Add a pervasive scalar field — and the black hole would grow "hair," becoming even more exotic, just like in this theory.

S = \frac{1}{16\pi} \int d^4x \sqrt{-g} \left( R - 2(\nabla \varphi)^2 + 2\lambda \varphi \, R^2_{GB} \right)
The scalar field φ couples to curvature via the Gauss-Bonnet invariant, adding a correction to standard Einstein gravity.
\chi^{BH}_{EsGB} = \chi^{BH}_{GR} + \chi^{BH}_{mod}
The total deflection angle is the sum of the GR prediction and an extra contribution from the scalar field, allowing precise computation of corrections.
Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole gravitational waves numerical simulation spacetime curvature gravity LIGO entropy Time dilation
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsLorentz transformations
Original: arXiv:2605.04224v1 · CC BY 4.0 · bridge42worlds