Simple

Dark Energy Didn’t Kick In Right Away ⚡ экспресс

Original: "When Dark Energy Turns On: Constraints on a Critical Emergence Model"
arXiv:2603.13137 · 2026-03-13 · CC BY 4.0 · ⏱ 1 min · Cosmology
Scientists tested a model in which dark energy only appears after a certain point in the universe’s history.
Abstract

Dark energy might not have existed from the very beginning, but "woke up" at a certain moment, like a volcano after dormancy. Scientists tested this idea with the latest cosmic data and found that it does not contradict observations so far, though it doesn’t solve all mysteries. What other secrets might the Universe be hiding in its history?

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Dark energy is usually seen as an innate property of the cosmos, at work from the very first moments. But a new model suggests it behaved like water on the verge of boiling: long unnoticed, then suddenly kicking in at a critical moment. This scenario is called 'late activation': around 5–7 billion years ago, a shift occurred, and the universe’s expansion began to accelerate.

Three landmarks helped test the idea. The cosmic microwave background—the cooled light of the Big Bang—preserved the imprint of the young universe. Explosions of supernovae, like lighthouses, allowed distances to be measured; it was these that led Adam Riess to discover the acceleration in the 1990s. The patterns of galaxies revealed the rate of universe expansion. By combining these data, scientists essentially captured the moment the cosmos 'boiled over.'

There was a surprise:

in a combination of cosmic microwave background and galaxy data, the 'late activation' model of dark energy turned out to be statistically more preferable than the standard one.

However, this doesn't resolve the main cosmological puzzle—the Hubble tension, i.e., the discrepancy in the expansion rate measured by different methods. The mystery endures, and cracking it will require even bolder ideas.

🎯 If dark energy had 'woken up' too early, just a couple of billion years after the Big Bang, the galaxies and stars we know simply wouldn’t have formed—the expansion would have scattered all matter.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy big bang supernova expansion of the universe
Laws
Friedmann equationsHubble's lawEinstein field equationsPlanck's lawChandrasekhar limitFermi acceleration
Original: arXiv:2603.13137 · CC BY 4.0 · bridge42worlds