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How long does a black hole live? A new answer from quantum physics ⚡ экспресс

Original: "Minimum lifetime of a black hole"
arXiv:2605.03922v1 · 2026-05-05 · CC BY 4.0 · ⏱ 1 min · General Relativity Cosmology HEP Theory
Scientists have figured out how long it takes for a black hole to completely disappear and return all the captured information.
Abstract

Imagine a black hole as a leaky bucket that slowly empties. Scientists calculated how long it takes for the bucket to 'cleanse' all the swallowed information. It turns out this process could take an unthinkably long time, possibly leaving behind a minuscule, barely oozing remnant. Could such remnants still be drifting through the universe?

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Black holes are not eternal: they slowly lose energy, emitting entropy — a measure of hidden information — as heat. This process was predicted by Stephen Hawking. But until now, it remained a mystery what happens at the very end, when the hole has almost disappeared and must return the captured data.

Now physicists have shown: after the main mass evaporates, a tiny white hole remains. Like a dying ember, it slowly releases information. The time for this 'cleanup' grows with the mass of the original black hole far more steeply than previously thought.

For a hole with the mass of a mountain, this time exceeds the age of the Universe by billions of times. But for microscopic holes, born during the Big Bang, the process could be finishing right now.

Perhaps we will be able to see the faint radiation from these remnants — maybe they are hiding under the mask of dark matter.

🎯 The complete evaporation time for a black hole with the mass of a mountain exceeds the age of the Universe by billions of times. And microscopic holes from the dawn of time may be burning out right now, and their last heat could be detected.

t_{\text{pur}} \sim M_0^4 / \hbar^{3/2}
The cleanup time of a black hole (t_pur) grows as the fourth power of its initial mass (M_0), divided by the Planck constant (ℏ) raised to the 3/2 power.
Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
black hole entropy dark matter big bang
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropy
Original: arXiv:2605.03922v1 · CC BY 4.0 · bridge42worlds