PROJECT SNO+ | DARKSIDE-50
>SNO+ is a multipurpose scintillator based neutrino experiment which is located 2km underground at SNOLAB, Creighton mine, Sudbury.
The primary physics goal of the experiment is the search for the elusive process of neutrino-less double beta decay with 130Te loaded into the liquid scintillator cocktail. In addition, SNO+ will be able to detect low energy solar neutrinos, geo- and reactor-antineutrinos, as well as supernova neutrinos. SNO+ has completed its water phase in 2019. During the water phase SNO+ made measurements of 8B neutrinos, and improved the limits on the lifetime of nucleon decay. Aside from the physics goals, the optical and energy calibration of the detector was accomplished in water phase. SNO+ has finished filling the detector in May 2022, and preparing for the 130Te phase.
>The __DarkSide__collaboration is an international affiliation of universities and labs seeking to directly detect dark matter in the form of weakly interacting massive particles (WIMPs). The collaboration is planning, building and operating a series of liquid argon time projection chambers (TPCs) that are employed at the Gran Sasso National Laboratory in Assergi, Italy. The detectors are filled with liquid argon from underground sources[1] in order to exclude the radioactive isotope 39
Ar, which makes up one in every 1015 (quadrillion) atoms in atmospheric argon.[2] The Darkside-10 (DS-10) prototype was tested in 2012, and the Darkside-50 (DS-50) experiment has been operating since 2013. Darkside-20k (DS-20k) with 20 tonnes of liquid argon is being planned as of 2019
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