Cosmogenic production of Ar in the context of the LUX-ZEPLIN experiment
arXiv:2201.02858 · doi:10.1103/PhysRevD.105.082004
Abstract
We estimate the amount of Ar produced in natural xenon via cosmic ray-induced spallation, an inevitable consequence of the transportation and storage of xenon on the Earth's surface. We then calculate the resulting Ar concentration in a 10-tonne payload~(similar to that of the LUX-ZEPLIN experiment) assuming a representative schedule of xenon purification, storage and delivery to the underground facility. Using the spallation model by Silberberg and Tsao, the sea level production rate of Ar in natural xenon is estimated to be 0.024~atoms/kg/day. Assuming the xenon is successively purified to remove radioactive contaminants in 1-tonne batches at a rate of 1~tonne/month, the average Ar activity after 10~tonnes are purified and transported underground is 0.058--0.090~Bq/kg, depending on the degree of argon removal during above-ground purification. Such cosmogenic Ar will appear as a noticeable background in the early science data, while decaying with a 35~day half-life. This newly-noticed production mechanism of Ar should be considered when planning for future liquid xenon-based experiments.
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Cited by in corpus (9)
- First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
- A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
- A search for new physics in low-energy electron recoils from the first LZ exposure
- New constraint on neutrino magnetic moment and neutrino millicharge from LUX-ZEPLIN dark matter search results
- Background Determination for the LUX-ZEPLIN (LZ) Dark Matter Experiment
- Reactor neutrino liquid xenon coherent elastic scattering experiment
- Study of cosmogenic activation above ground for the DarkSide-20k experiment
- Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data
- Search for New Physics via Low-Energy Electron Recoils with a 4.2 Tonne\times Year Exposure from the LZ Experiment