Simple

Death of a Black Hole: Not Disappearance, but a Tear in the Fabric of the Universe

Original: "Breakdown of Semiclassical Gravity in Four-Dimensional Black Hole Evaporation"
· David A. Lowe, Larus Thorlacius
arXiv:2605.00780v1 · 2026-05-01 · CC BY · ⏱ 1 min · HEP Theory General Relativity
Computer modeling reveals: as they evaporate, black holes tear the very fabric of spacetime.
Abstract

Scientists have found out: during the birth and evaporation of black holes, a sudden tear in spacetime — a ‘thunderbolt’ — can appear far from the hole, where everything is calm. Like a tiny crack that causes a dam to burst far downstream, this challenges our usual ideas about the fate of information in black holes.

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A black hole is like a fabric stretched to its limit, holding everything around it. Stephen Hawking showed that it still loses mass: particles slip away like threads from a worn-out cloth. It seemed the finale would be quiet—just a disappearance.

But a computer simulation revealed a catastrophe. When the hole runs out, the fabric of spacetime doesn't smooth out but rips apart. An instantaneous rupture—a 'thunderbolt'—travels at the speed of light, tearing even calm regions. This is not a silent fading but a cosmic rending.

Hence, our theories break down at the very edge. The debate over the fate of information that falls in remains unresolved—perhaps a future theory will bring the answer. The irony is that Hawking introduced the term 'thunderbolt' in 1993 as a hypothetical quirk, and today modeling confirms its inevitability. Incidentally, Bekenstein already guessed that a black hole has entropy (a measure of disorder), and Unruh developed similar ideas.

🎯 Hawking coined the term 'thunderbolt' in 1993 as a hypothetical curiosity, not believing it was real; modeling proved otherwise.

ds^2 = -e^{2\rho} du dv + r^2 d\Omega^2
Spacetime geometry: u and v are retarded and advanced time, r is the radial coordinate determining the area of the 2-sphere.
K = R_{\mu\nu\lambda\rho} R^{\mu\nu\lambda\rho}
Invariant measure of curvature: sum of squares of all components of the Riemann tensor; shows how strongly spacetime is curved at each point.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterNiels Bohr
Tags
black hole spacetime curvature Quantum Field numerical simulation entropy quantum information Time dilation redshift uncertainty principle speed of light
Laws
second law of thermodynamicsDoppler effectHeisenberg uncertainty principleHawking radiationgravitational lensingprinciple of constancy of the speed of light
Original: arXiv:2605.00780v1 · CC BY · bridge42worlds