Direct Proof of Dark Matter May Lurk at Low-Energy Frontiers
Even after decades of searching, scientists have never seen a particle of dark matter. Evidence for the substance’s existence is close to incontrovertible, but no one yet knows what it is made of. For decades physicists have hoped dark matter would prove to be heavy—consisting of so-called weakly interacting massive particles (WIMPs) that could be straightforwardly detected in the lab.
With no definitive sign of WIMPs emerging from years of careful searching, however, physicists have been broadening the scope of their quest. As new, more precise experiments ramp up data collection, researchers are reassessing theories about how dark matter particles lighter than a proton might appear in their detectors. Two papers posted on the preprint server arXiv.org earlier this year are emblematic of these shifting sensibilities. They are the first to propose that a detector could find plasmons—aggregates of electrons moving together in a material—produced by dark matter.
The first study was conducted by a group of dark matter researchers at the Fermi National Accelerator Laboratory (Fermilab) in Batavia, Ill., the University of Illinois at Urbana-Champaign and the University of Chicago. They propose that low-mass dark matter could produce plasmons—which they claim some detectors may already be seeing. Inspired by that first paper, physicists Tongyan Lin and Jonathan Kozaczuk, both at the University of California, San Diego, calculated how likely low-mass dark matter is to generate plasmons in a detector.