Latest Results on Direct Detection of Dark Matter WIMPs - IceCube 2025

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Researchers use large, sensitive detectors located deep underground to directly search for the dark matter particles that may continually pass through the Earth. Researchers can also search for dark matter indirectly through specific signatures in cosmic rays and gamma rays.
One particular galaxy cluster, known as the Bullet Cluster, provides some of the best evidence we have for the existence of dark matter. This cluster is made up of two smaller clusters that collided sometime in the past.
IceCube detects light emitted by charged particles that are produced when a single neutrino crashes into a proton or neutron inside an atom. The resulting nuclear reaction produces secondary particles traveling at high speeds (faster than light in the ice!) that give off a blue light called Cherenkov radiation.
Neutrino Physics. IceCube has recorded an unusually large set of neutrinos. From over ten years data, we have accumulated about 700,000 between 100 GeV and 1 PeV and 200,000 between 10 GeV and 100 GeV. Both datasets have outstanding purity, at more than 99% with respect to downgoing cosmic ray muons.
We compare our model projections with the most current constraints and show that the IceCube detector can detect CR-boosted dark matter especially with masses below when scattering with electrons and in the nucleon scattering case.
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One of the only experiments to detect axions as dark matter is the Axion Dark Matter Experiment (ADMX). Located at the University of Washington, ADMX uses a resonant microwave cavity in a strong magnetic field to convert dark matter into microwave photons by means of the Primakoff effect.
Direct detection of dark matter is based upon the premise that since it is known that dark matter exists in some form, Earth must intercept some as it carves out a path through the universe. Direct detection experiments attempt to create highly sensitive systems capable of detecting these rare and weak events.
IceCube detects high-energy neutrinos using the Cherenkov light produced by relativistic charged particles that result from the interaction of these neutrinos with the atomic nuclei of Antarctic ice.

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