For nearly five decades, scientists were unable to measure thorium-229’s resonance frequency with enough precision to build a nuclear clock, but last year brought two major advances. First, a group at the National Metrology Institute of Germany (PTB) published relatively accurate measurements. A few months later, a team from the University of Colorado released results that were several million times more precise.
“We still need even greater precision to develop a nuclear clock,” says Perez, “but we’ve already identified an opportunity to study dark matter.” He explains: “In a universe made up only of visible matter, the physical conditions and the absorption spectrum of any material would remain constant. But because dark matter surrounds us, its wave-like nature can subtly change the mass of atomic nuclei and cause temporary shifts in their absorption spectrum. We hypothesized that the ability to detect minute deviations in the absorption spectrum of thorium-229 with great precision could reveal dark matter’s influence and help us study its properties.”
Theoretical calculations made by the team – led by Dr. Wolfram Ratzinger from Perez’s group and other postdoctoral fellows – showed that the new measurements could detect dark matter’s influence even if it were 100 million times weaker than gravity, a force that is itself weak and rarely crosses our minds in daily life. “This is a region where no one has yet looked for dark matter,” says Ratzinger. “Our calculations show that it’s not enough to search for shifts in the resonance frequency alone. We need to identify changes across the entire absorption spectrum to detect dark matter’s effect. Although we haven’t found those changes yet, we’ve laid the groundwork to understand them when they do appear. Once we detect a deviation, we’ll be able to use its intensity and the frequency at which it appears to calculate the mass of the dark matter particle responsible. Later in the study, we also calculated how different dark matter models would affect thorium-229’s absorption spectrum. We hope this will ultimately help determine which models are accurate and what dark matter is actually made of.”