Simple

How the Universe Became Smooth: Unraveling the First Moments ⚡ экспресс

Original: "A novel pre-inflationary model in view of the lack of angular correlation of CMB"
arXiv:2605.20076 · 2026-05-19 · CC BY · ⏱ 1 min · General Relativity Cosmology HEP Theory Space Physics
A new model explains why the oldest cosmic map lacks large spots.
Abstract

Scientists proposed a model where the universe before inflation first expanded slowly, then abruptly accelerated—like a car easing into motion before rapidly gaining speed. This explains why the cosmic microwave background is surprisingly uniform on the largest angular scales. This 'warm-up' before the Big Bang left a noticeable imprint on the cosmos. What if the birth of the universe had a preface?

Links in the knowledge graph 1

The birth of the universe resembles not an explosion, but a traffic jam. At first, a tiny fraction of a second after the Big Bang, space expanded sluggishly, like cars stuck in gridlock. Then came a sharp surge—accelerated expansion, which cosmologists call inflation. This contrasting transition explains an ancient mystery: why there are no large spots in the snapshot of the universe's microwave 'echo.' The slow phase acted like a filter, preventing large energy fluctuations from growing. Only fine ripples remained—the very quantum jolts from which galaxies later emerged. Remarkably, without such a jam, the familiar cosmos might never have formed: all matter would have collapsed into giant black holes or remained a diffuse fog. The new model, consistent with Planck satellite data, was developed by Alan Guth and others. Yet back in the 1940s this 'echo' was predicted by George Gamow, and in 1965 it was serendipitously detected by Arno Penzias and Robert Wilson.

🎯 A delay in the first minuscule fraction of a second shaped the cosmos: without this 'cosmic traffic jam,' stars might never have ignited at all.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
big bang expansion of the universe Standard Model
Laws
Friedmann equationsHubble's lawNoether's theoremEinstein field equationsPlanck's lawspin–statistics theorem
Original: arXiv:2605.20076 · CC BY · bridge42worlds