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Helium Hydride Ion Retains Cooling Power in Early-Universe Simulation

Experiments at Heidelberg’s Cryogenic Storage Ring confirmed that helium hydride ions stayed reactive at near-absolute-zero temperatures, revealing their underestimated cooling impact on primordial gas.

A bright light with a halo around it.
ames Webb Space Telescope’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust.
© NASA & ESA

Overview

  • MPIK researchers stored HeH⁺ ions at a few kelvins in the Cryogenic Storage Ring and collided them with deuterium to replicate conditions just after the Big Bang.
  • Measured reaction rates of HeH⁺ with hydrogen isotopes remained nearly constant down to a few kelvins, overturning prior predictions of steep declines at low temperatures.
  • A theoretical team led by Yohann Scribano identified and corrected an error in the potential energy surface, bringing calculations into close agreement with experimental results.
  • Sustained HeH⁺ reactivity implies a stronger role in catalyzing molecular hydrogen formation and dissipating heat during the cosmic dark ages.
  • These findings prompt revisions to primordial chemistry models and simulations of Population III star formation by highlighting a more critical cooling function for HeH⁺.