Particle.news

Download on the App Store

HeH+ Ion’s Reactivity Endured at Cryogenic Temperatures, Reframing Early-Star Cooling

Corrected theoretical models now align with collision data under cryogenic conditions, revealing HeH+’s sustained reactivity enabled primordial gas to cool.

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

  • Researchers at MPIK used the Cryogenic Storage Ring to trap HeH+ ions at a few kelvins and collide them with beams of neutral hydrogen and deuterium atoms.
  • Collision rates remained nearly constant down to ultra-low temperatures, overturning long-standing predictions of a slowdown in HeH+ reactivity.
  • A team led by Yohann Scribano uncovered and fixed an error in previous potential energy calculations, bringing theoretical models into agreement with experimental results.
  • The persistence of HeH+ reactivity suggests it played a more significant role as a coolant in early-universe gas clouds, aiding the collapse of protostars.
  • Findings published in Astronomy & Astrophysics refine our understanding of primordial chemistry and molecular cooling mechanisms that enabled the first stars to form.