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Dark Energy: How a New Survey Changes the Picture ⚡ экспресс

Original: "Evidence for evolving dark energy from DESI DR2 BAO and Pantheon$$^+$$, DES-Dovekie, and Union3"
arXiv:2508.10514 · 2025-08-14 · CC BY · ⏱ 1 min · Cosmology General Relativity HEP Theory
A map of millions of galaxies hints: dark energy may be changing its strength. This threatens the Universe with a different end.
Abstract

Dark energy is a mysterious force that makes the Universe expand faster and faster. Scientists checked whether it has changed over time using the latest galaxy map (DESI) and supernova data. Hints of change exist, but they are too faint and uncertain, like a whisper in a noisy room. Maybe dark energy does evolve, but is the cosmos playing hide-and-seek with us?

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For almost a hundred years, astronomers have known that galaxies are flying apart. But in the 1990s, observations of supernova explosions revealed: this is happening faster and faster. The cause was dubbed dark energy — an invisible force inflating space. The discovery earned the Nobel Prize for Солу Перлмуттеру, Адаму Риссу, and Брайану Шмидту. Since then, scientists have been trying to figure out whether this cosmic 'gas pedal' is constant.

The new DESI survey mapped millions of галактик and tracked their motion via imprints of density waves from the Big Bang era. Combined with data on сверхновых, this indicated: тёмная энергия may be neither eternal nor uniform. It sometimes weakens, sometimes strengthens — like an engine that changes its own revs. A model called Mirage gave the clearest signals, but what's more surprising: if this trend holds true, the Universe is destined not for eternal расширение but for a rip — when space itself starts tearing apart galaxies and atoms.

The statistical significance is still low — 2 sigma, like flipping seven heads in a row. We're far from a reliable 5 sigma. Yet each new sky map brings the answer closer: either dark energy is an unchanging property of the vacuum, or a living, evolving entity. And on this hinges whether the cosmos freezes in eternal cold or vanishes in a fiery flash.

🎯 Dark energy makes up about 70% of the Universe's mass-energy. If it isn't constant, the cosmos may end in a rip, not a freeze.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy supernova galaxy expansion of the universe
Laws
Friedmann equationsHubble's lawvirial theoremChandrasekhar limitFermi accelerationlaw of conservation of momentum
Original: arXiv:2508.10514 · CC BY · bridge42worlds