Dark Energy as a Quantum Effect express

Original: "Cosmological Constraints on the Generalized Uncertainty Principle from Redshift-Space Distortions"
· Andronikos Paliathanasis
arXiv:2604.01713 · 2026-04-02 · CC BY 4.0 · 1 min
The accelerated expansion of the Universe is a consequence of quantum 'graininess' of space.

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If space is a canvas, then brushstrokes cannot be infinitely thin. There's a tiniest segment, shorter than which there's no point in measuring. This quantum 'graininess' alters the geometry itself: the motion of galaxies and the growth of large-scale structures bear its mark.

Scientists replaced the mysterious dark energy with such a correction and derived an equation for the expansion of the Universe. The model was compared with data: supernova supernovae (the Nobel triumph of Adam Riess) and the echo of the Big Bang.

It turned out that the graininess parameter is negative — as if space itself were 'pushing' matter apart, accelerating the expansion.

This quantum picture is not inferior to the standard model, and in a number of tests even outperforms it. It seems that dark energy is not a new substance, but a shadow of the quantum world cast on cosmic scales.

Original abstract

as written by the authors arXiv:2604.01713

We investigate the imprints of the Generalized Uncertainty Principle on cosmological scales by using redshift-space distortion measurements in combination with background cosmological data to determine constraints on the deformation parameter $$\beta$$. We consider the modified Poisson bracket related to the existence of a minimal length, which leads to a modified Raychaudhuri equation for the standard $$\Lambda$$CDM model and gives rise to a phenomenological one-parameter dynamical dark energy scenario. Through this modification, we can reveal the effects of the minimal length on the late-time structure of the universe. We employ the $$f$$ and $$f\sigma_8$$ measurements of the growth rate combined with background data, including cosmic chronometers, baryon acoustic oscillations and Type Ia supernova observations. The observational constraints reveal a systematically negative value for the deformation parameter $$\beta$$, with the $$\Lambda$$CDM limit lying within the 95\% credible interval. When supernova data are included, the Akaike Information Criterion indicates weak-to-strong support in favour of the GUP-modified model depending on the SNIa catalogue, while the Bayesian evidence suggests a weak preference.

A ruler that never shows less than a millimeter is the essence of the uncertainty principle with a minimum length: it's impossible to measure distance with infinite precision.

Scientists
George GamowLeo EsakiWilliam UnruhVera RubinFritz ZwickyAdam Riess
Concepts
cosmological parameters cosmic expansion uncertainty generalized uncertainty principle cosmological data Cosmic Censorship Principle constraint lambda cdm ecdm model sigma 8 dark energy alternatives newtonian limit density contrast chi squared minimisation perturbation spectrum gravitational constant equation of state parameter standard quantum limit dark energy measurement hubble constant cosmic distance measurement