Light Delay Near Black Holes Will Uncover the Mystery of Dark Matter express

Original: "Strong-lensing degeneracies of black holes embedded in self-interacting scalar field dark matter halos"
· Mohsen Fathi, Gabriel Gómez
arXiv:2605.27242 · 2026-05-26 · CC BY 4.0 · 1 min
The way a black hole bends light barely depends on its surroundings, but precise clocks will reveal how much invisible matter lurks.

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The gravity of a black hole creates a curvature of spacetime, acting like a lens: light from a distant galaxy splits in two, stretching into arcs. Dark matter around the hole barely changes the picture, as if a transparent curtain was added to a window pane. But light from the different images arrives with a delay — from minutes to years. And it's this interval that slightly shifts due to the invisible substance.

Calculations show: even for giant holes, the image distortion is less than a thousandth of a percent. However, the arrival time difference of the 'twins' shifts by fractions of a second — atomic clocks can notice such a thing.

A supernova flash, looping around the black hole from different sides, reaches us with an interval of years. Dark matter adds a tiny pinch to this interval, but a measurable one.

Time becomes the key to the invisible halo. And although image distortions are negligible, future telescopes will catch microsecond shifts. Paradox: the delay from the hole itself can be so gigantic that the light set off before the first humans appeared on Earth.

In 1912, Albert Einstein predicted that gravity bends light; the first mirage ring was found only in 1979 with the help of radio telescopes.

In 'Interstellar', the heroes study the black hole Gargantua by the distorted light of stars — the scene almost exactly mirrors the calculations for the real M87*.

Scientists
Fritz ZwickyVera RubinJacob BekensteinKarl SchwarzschildStephen HawkingSubrahmanyan Chandrasekhar
Concepts
black hole photon ring black hole light bending dark matter lensing strong lensing dark matter subhalo photon sphere strong gravitational field schwarzschild metric host galaxy inner horizon effective spin milky way halo structure apparent horizon logarithmic correction EHT Hawking area theorem area law halo scalar perturbations schwarzschild radius