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Dark Energy That Will Disappear express

Original: "Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations"
arXiv:2606.05723 · 2026-06-04 · CC BY · 1 min · Cosmology
The MEDE model treats dark energy not as an eternal force, but as a temporary tailwind: it emerged when the Universe was half its age, and will gradually fade away, explaining puzzling fluctuations in its behavior.
Abstract

The Metastable Emergent Dark Energy (MEDE) model extends phenomenological models PEDE and GEDE, introducing transient behavior: dark energy appears at late times and fades into the future. The equation of state is given by w(z) = -1 - Δ tanh[log10((1+z)/(1+z_t))], with two free parameters: z_t — the transition redshift, and Δ — the amplitude of variation. Constraints from a joint analysis of Planck CMB, DESI DR2 BAO, and supernova compilations (including PantheonPlus) yield z_t = 0.425+0.084−0.120 and Δ = 0.87+0.29−0.35, indicating a statistically significant deviation from the cosmological constant. Comparison of information criteria shows a preference for MEDE over ΛCDM (ΔDIC = -9.29) and comparability with the CPL parametrization (ΔDIC = 0.74). The model retains the success of ΛCDM in describing the early Universe and naturally explains the crossing of the phantom divide in low-redshift data.

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Since the late 20th century, astronomers have known that the recession of galaxies is accelerating, as if pushed by an invisible tailwind. This mysterious force was dubbed dark energy and long thought to be a steady, unchanging breeze — for its discovery, Adam Riess and Saul Perlmutter were awarded the Nobel Prize.

The MEDE model breaks this canon: dark energy is not an eternal wind, but a temporary gust that arose when the Universe had lived half its current age. Two simple numbers — the moment of appearance and the strength of the pull — fully define its character. Comparison with data from distant stellar explosions and the afterglow of the Big Bang revealed something unexpected: this 'scheduled wind' aligns with reality better than the classical, undiminishing tug. Moreover, this gust is not perfectly smooth: its strength apparently fluctuated, crossing a mysterious threshold where pressure begins to exceed energy, and MEDE naturally explains such jumps.

The most intriguing part — in the future, this gust will die out, and the expansion of the cosmos will continue by inertia, like a bicycle that's no longer being pedaled. The irony is that the greatest force accelerating the Universe turns out to be just an episode.

🎯 If the model is correct, in the distant future dark energy will disappear, and the expansion of space will continue only due to the accumulated momentum.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark energy expansion of the universe supernova big bang
Laws
Friedmann equationsHubble's lawEinstein field equationsPlanck's lawChandrasekhar limitFermi acceleration
Original: arXiv:2606.05723 · CC BY · bridge42worlds