SCIENCE

How JWST puts the squeeze on light dark matter, for free | by Ethan Siegel | Starts With A Bang! | Mar, 2025

Although the Spitzer space telescope’s infrared views could reveal many features, such as the warped disk, within the Sombrero galaxy, the superior size, resolution, and wavelength capabilities of JWST show a large set of features that Spitzer simply couldn’t resolve. The scientific gains, as well as visual ones, are there for us all to reap, with the “blank sky” regions of JWST’s views returning additional science about the presence of “extra” photons that could result from dark matter-driven processes. (Credits: NASA/JPL-Caltech/University of Arizona/STScI & NASA, ESA, CSA, STScI)

One of the most promising dark matter candidates are light particles, like axions. With JWST, we can rule out many of those options already.

All throughout the Universe, there’s a massive puzzle whose solution remains unknown: the dark matter mystery. Within every large, high-mass system that we examine, including:

  • spiral galaxies,
  • elliptical galaxies,
  • groups of galaxies,
  • clusters of galaxies,
  • cosmic filaments,
  • and the large-scale cosmic web,

there simply isn’t enough normal matter to explain the gravitational signals we observe. From the internal motions of galaxies to the relative motions of galaxies within a cluster to the gravitational lensing signals generated by these objects to the clustering patterns of galaxies on the largest of cosmic scales, some novel type of mass that neither absorbs nor emits light — dark matter — must be present to consistently explain what we observe.

And yet, all of our efforts to directly detect dark matter have come up empty, with key signals from particle colliders, cosmic ray experiments, and possible signatures of…


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