How Quantum Chaos Gives Rise to Inflation ✎ express

Original: "From Quantum Correlations to Inflationary Tracking Scalar Field Evolution"
· V. K. Oikonomou
arXiv:2608.01165v1 · 2026-08-02 · arXiv non-exclusive · independent analysis · 1 min
Scientists have shown that the early universe, being a quantum chaos, created on its own the scalar field that inflated it to gigantic sizes.

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The early universe resembled an overheated cauldron, seething with quantum fluctuations (random bursts of energy). In this chaos, like steam over boiling water, a special field, the scalar field, condensed. It became the 'engine' that made space expand at an incredible rate. This process is called inflation.

The authors showed that such a field need not be introduced artificially. It arises on its own, as a collective behavior of many quantum particles. Using ideas from statistical physics and quantum field theory, they derived the condition under which expansion proceeds exactly as observed in the cosmic microwave background. This condition links the rate of change of the field to the expansion rate.

The cosmic microwave background is the 'echo' of the Big Bang, reaching us after 13.8 billion years. It is studied using satellites such as 'Planck' and ground-based telescopes.

This approach turns inflation from a hypothesis into a consequence of the quantum nature of the universe. The entire observable universe is but foam left after the quantum 'cauldron' spilled its contents into the classical world.

Inflation lasted a tiny fraction of a second, but during that time the universe expanded by a factor of $10^{26}$—as if a grain of sand became the size of a galaxy.

\dot{\phi}^2 = \gamma H^{-m}
The rate of change of the scalar field is related to the Hubble parameter H (expansion rate) and constants γ, m.
Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
multi field inflation inflaton inflationary cosmology stochastic inflation refined inflationary dynamics cosmological collider scalar field scalar radiation de sitter space global warming quantum nature of gravity plasma heating spatial curvature classical physics potential reheating Fisher's equation Friedmann equations inflationary gravitational waves expanding universe