How to Make a Black Hole Perfectly Black ✛ ✎

Original: "Total absorption of tailored incoming signals by black holes"
arXiv:2509.19451 · 2025-09-23 · arXiv non-exclusive · independent analysis · 1 min
By shaping incoming space ripples, scientists forced a black hole to absorb all energy, rendering it truly black.

Black holes typically reflect a portion of the ripples in space called gravitational waves, like a bell that doesn't ring purely when struck. Physicists discovered that by precisely shaping these waves to match the black hole's natural resonance, they can make it absorb all the energy, becoming perfectly black and silent during the impact. The energy is stored momentarily.

Then, the black hole releases the energy as a clean, ringing tone. Like the ring of a bell reveals its exact shape, this echo carries detailed information about the black hole's inner structure. Curiously, while in this perfectly absorbing state, the black hole would be completely invisible, detectable only by its gravitational pull on nearby stars. This opens a new way to probe the spacetime curvature around these objects.

The trick is so delicate that even a tiny mismatch in the wave shape breaks the perfect absorption, causing the black hole to reflect energy again.

This concept mirrors the 'singularity drives' of science fiction, which store and release energy in controlled bursts.

\omega_n = \sqrt{\frac{n^2 \pi^2}{4L^2} + V_0}
Discrete set of real frequencies at which reflection from the barrier vanishes
2i\omega_{VA} \sqrt{\omega_{VA}^2 - V_0} = -V_0 \sin\left(2\sqrt{\omega_{VA}^2 - V_0} L\right)
Transcendental equation determining the complex frequencies of virtual absorption
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyKarl SchwarzschildSubrahmanyan ChandrasekharRainer Weiss
Concepts
black hole evaporation black hole accretion wave amplification information loss accretion disk wind gravitational wave echoes quasar feedback light absorption quasinormal modes ringdown gravitational singularity scalar perturbations topological transition remnant holography naked singularity tidal disruption event traversable wormhole Hawking radiation black hole