Dark Energy Isn't Constant? ✎ express

Original: "Breaking Free from the Swampland of Impossible Universes through the DESI Portal"
· Luis A. Anchordoqui, Dieter Lust
arXiv:2605.10476 · 2026-05-11 · arXiv non-exclusive · independent analysis · 1 min
Observations of millions of galaxies hint that dark energy, the “yeast” of the Universe, might be weakening over time.

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For a long time, dark energy, the mysterious force prodding the expansion of the Universe, was considered eternal and unchanging, like yeast that never loses its activity. But explaining such constancy through the laws of the microcosm proved impossible, and scientists began to suspect that the “leaven” might be going flat.

In 1998, Adam Riess, Saul Perlmutter, and Brian Schmidt proved that the Universe is expanding at an accelerating rate, earning the Nobel Prize.

The DESI instrument, a light analyzer of millions of distant galaxies, showed that over the past few billion years, dark energy’s strength has weakened by about 10%. By studying galaxy distributions, astronomers were surprised to find that they are not scattered randomly but arranged in concentric rings, like ripples on water from a thrown stone. This is the frozen echo of sound waves that shook the early Universe.

Now the entire recipe of the cosmic loaf is in question, where dark matter and dark energy were considered immutable ingredients. Cosmologists are trying out new recipes where the dough of space is kneaded with string-like filaments, and dark energy, like live yeast, behaves capriciously: sometimes raging, sometimes quieting down, promising a dramatic finale to the expansion.

By some estimates, dark energy makes up about 68% of all the energy in the Universe.

Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesFritz Zwicky
Concepts
cosmological constant problem desi lambda cdm vacuum energy ecdm model de sitter space cold dark matter cosmological constant dark energy alternatives cosmic string anti de sitter space false vacuum interaction model equation of state parameter dilaton cosmic distance measurement quintessence string theory lcdm model dark energy