Uno studio recente condotto da Richard Schnee, un professore di fisica della Syracuse University, pubblicato sulla rivista online Symmetry, tenta di far luce sulla natura e origine della materia scura, quella componente elusiva che costituisce quasi il 27% del contenuto materia-energia dell’Universo, considerando la possibilità di eseguire una serie di esperimenti che permettano di trovare degli indizi su quelle eventuali particelle che non sono molto pesanti.
“Scientists looking for dark matter face a serious challenge, in that no one knows its properties”, says Schnee, also principal investigator of the Cryogenic Dark Matter Search (CDMS) Physics Lab at SU. “Experiments have seen no signs of dark matter particles that have high masses, but a few experiments have claimed hints of possible interactions from dark matter particles with low masses”. An expert in particle physics, Schnee hopes to find traces of dark matter with an experiment that is more sensitive to such low-mass dark matter particles. His group is part of a multinational team of scientists working on SuperCDMS, an experiment in the University of Minnesota’s Soudan Underground Laboratory that is designed to detect dark matter. Although dark matter has never been seen directly, it is thought to be six times more prevalent in the universe than normal matter. “Everywhere we look, objects are accelerating due to gravity, but the acceleration is too large to be caused by only the matter we see”, Schnee says. “Even more remarkably, we can infer that this extra dark matter is composed not of normal atoms, but other kinds of particles”. Scientists believe the mystery particles are WIMPs (Weakly Interacting Massive Particles), which travel at hundreds of thousands of miles per hour through space and shower the Earth on a continuous basis. Unlike normal matter, WIMPs do not absorb or emit light, so they cannot be viewed with a telescope. “Spotting the occasional WIMP that interacts with something is extremely challenging because particle interactions from natural radioactivity occur at a much higher rate. Detecting a WIMP is like spotting a needle in a haystack”, Schnee continues. Enter CDMS, whose hypersensitive detectors can differentiate between rare WIMP interactions and common ones involving radioactivity. The size of a hockey puck, a CDMS detector is made up of a semiconductor crystal of germanium that, when cooled to almost absolute zero, can detect individual particular interactions. The presence of layers of Earth, like those at the Soudan lab, provide additional shielding from cosmic rays that otherwise would clutter the detector, as it waits for passing dark matter particles. “We cool our detectors to very low temperatures, so we can detect small energies that are deposited by the collisions of dark matter particles with the germanium”, says Schnee. “Other materials, including argon, xenon and silicon, are also used to detect low-mass dark matter particles. We need to consider as many materials as possible, along with germanium”. SU is one of 14 universities working collaboratively in the search for WIMPs. In the Physics Building, Schnee and his team have constructed an ultra-low radon “clean room,” in hopes of reducing the number of interactions from radioactivity that look like WIMPs. (Alpha and beta emissions from radon, a type of radioactive gas, can mimic WIMP interactions in a detector.) “Unfortunately, radon is all around us, so, even with this ‘clean room,’ some radon-induced interactions will still mimic WIMPs“, Schnee says. “All of us are building different types of detectors and are constantly improving our methods, in hopes of spotting WIMP interactions”.
Syracuse University: SU Plays Key Role in Search for Elusive Dark Matter arXiv: Introduction to dark matter experiments arXiv: Search for Low-Mass WIMPs with SuperCDMS