The DMRadio suite is MIT's phased plan to cover axion masses below 1 μeV. All phases use the same core principle — a strong magnetic field converts axions into a detectable electromagnetic signal — but at increasing scale and sensitivity.
Jessica Fry is a 5th-year physics PhD candidate at MIT's Laboratory for Nuclear Science, building specialized detectors for the DMRadio program. She has an unusual background — she was a professional Broadway performer before switching to physics. MIT's spotlight describes her transition as "from the Broadway stage to MIT's Laboratory for Nuclear Science." She says of the axion hunt: "It's a hard problem. But it's a tractable one. It is a fun hunt" . Fry was named to the Forbes 30 Under 30 – Science (2026) list for her work leading the search for dark matter
. She has published 10 papers with nearly 200 citations
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BabyIAXO is an intermediate-stage "axion helioscope" that will search for axions produced in the Sun. It uses a custom superconducting dipole magnet — described by project coordinator Professor Matthias Schott of the University of Bonn as "the largest dipole magnet that's ever been constructed in particle physics" . The magnet is 10 m long with two 70 cm-diameter bores, operated at about −270°C and mounted on a moving platform to track the Sun for 12 hours a day
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The German Research Foundation (DFG) recently approved 6 million euros in funding through the Excellence Cluster "Color meets Flavor" at the Universities of Bonn, Siegen, and Dortmund to build the magnet system, which is now moving into construction . BabyIAXO is sited at DESY in Hamburg and will test the magnet, optics, and detector technologies for the full-scale International Axion Observatory (IAXO), which would have dramatically greater sensitivity to solar axions
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The field is growing rapidly and there is genuine optimism, but "inevitable" is stronger than the evidence supports. Multiple experiments — ADMX, CAPP, HAYSTAC, ABRACADABRA, and others — have steadily narrowed the allowed parameter space. DMRadio-m³ and ADMX-EFR are poised to probe the most theoretically well-motivated QCD axion models (KSVZ and DFSZ) in the coming years . Many physicists involved describe the hunt as a "tractable" problem with a distinctive predicted signal
. However, no axion signal has been detected yet, and the axion mass could lie in regions that remain experimentally challenging. The mood is best described as guarded optimism — the tools are finally arriving that could either discover the axion or definitively exclude it across wide ranges of mass, which would be a major result either way.