A faint glow from the early universe could help solve the mystery of dark energy
AI-summarised brief · reviewed before publication
Researchers announced that the Canadian Hydrogen Intensity Mapping Experiment (CHIME) can directly detect the faint radio glow of neutral hydrogen from the early universe, providing a new, cost‑effective method to study dark energy. By mapping hydrogen’s distribution without relying on external galaxy surveys, CHIME captured a signal from 5 billion years after the Big Bang using 94 nights of 2019 data, finding that about 2 % of hydrogen was neutral at that epoch. The instrument, built to probe cosmic expansion, now aims to trace hydrogen back to 3 billion years post‑Big Bang with its seven‑year dataset. The findings, detailed in two papers in The Astrophysical Journal, represent a milestone for Canadian‑led cosmology and open a novel avenue for testing models of galaxy formation and the accelerating universe.
💡 Why It Matters
- · Direct hydrogen mapping offers an unprecedented, independent probe of the large‑scale structure that drives dark‑energy measurements, potentially tightening constraints on its nature.