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Quantum Trick Accelerates the Universe Without Dark Energy ⚡ экспресс

Original: "A post-selected quantum model of cosmic acceleration"
arXiv:2606.12297 · 2026-06-10 · CC BY 4.0 · ⏱ 1 min · General Relativity Cosmology Quantum Physics
The universe is expanding faster and faster — possibly due to a quantum rule, not mysterious dark energy.
Abstract

An alternative explanation for cosmic acceleration is proposed, rooted in quantum post-selection—a standard quantum procedure typically ignored in cosmology. Instead of initial-condition models, we construct a minimal predictive model where post-selection and coarse-graining create an effective late-time acceleration, with no cosmological constant or modifications to general relativity. The expansion history is theoretically tight, adding at most two parameters beyond standard Friedmann evolution. Fitting to Type Ia supernovae and cosmic chronometer data gives statistically competitive results and naturally dodges the coincidence problem. The model mirrors standard behavior in the radiation- and matter-dominated eras and predicts a jerk parameter today that sharply differs from ΛCDM. The findings hint that cosmic acceleration might be a macroscopic quantum phenomenon.

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Since the end of the 20th century, we've known: the expansion of the Universe is accelerating — galaxies are flying apart faster and faster. The discovery brought a Nobel Prize to Adam Riess, Saul Perlmutter, and Brian Schmidt. The standard explanation relies on dark energy — an invisible force pushing space apart. New work proposes a different mechanism: it's all about post-selection — a quantum rule, like a detective story with a known ending where the clues are fitted to match it. The future selects only those event scenarios that lead to the desired outcome. This solves a longstanding mystery: why acceleration started just now, when both we and galaxies exist. The model introduces no mysticism and fits perfectly with data on supernovae and the age of galaxies. It also correctly describes the early epochs after the Big Bang. An unexpected conclusion: without such 'fitting,' acceleration would have started in an era of mere atoms — and stars would never have ignited.

🎯 Type Ia supernovae are stellar explosions with nearly identical power: they are used as standard 'rulers' to measure distances over billions of light-years.

🎬 Post-selection resembles the plot of Ted Chiang's story 'Story of Your Life,' where knowledge of the future determines actions in the present.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
expansion of the universe dark energy supernova big bang
Laws
Friedmann equationsHubble's lawEinstein field equationsPlanck's lawChandrasekhar limitFermi acceleration
Original: arXiv:2606.12297 · CC BY 4.0 · bridge42worlds