4.4 Article

Performance of the Li6Eu(BO3)3 crystal as a scintillating bolometer for studies of rare processes

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ELSEVIER
DOI: 10.1016/j.nima.2022.167549

Keywords

Li6Eu(BO3)(3) single crystal; Scintillator; Scintillating bolometer; Luminescence; Light yield; Quenching factor; Radiopurity

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In this study, we investigated the internal radioactive and chemical contamination of the Li6Eu(BO3)(3) scintillating crystal used as a cryogenic scintillating bolometer. The detector exhibited excellent discrimination power, effectively distinguishing beta/gamma events from alpha events. The crystal showed weak activity from daughter nuclides of U/Th chains, but significant contamination from the alpha-active nuclide Sm-147 was observed. The findings provide insights into the light yield and quenching factor for different particles, making the Li6Eu(BO3)(3)-based cryogenic scintillating bolometers attractive for various applications.
In this article we report on a detailed study of the internal radioactive and chemical contamination of the Li6Eu(BO3)(3) scintillating crystal operated as a cryogenic scintillating bolometer over 359 h. The excellent discrimination power of the detector allows to distinguish effectively beta/gamma events from alpha events. Whilst a weak activity of daughter nuclides from U/Th chains at the level few mBq/kg was observed, this crystal was found to be significantly contaminated by Sm-147, an alpha-active nuclide, at the level of about 0.5 Bq/kg. The light yield for beta/gamma events was determined to be 7.4(6) keV/MeV. The light yield and quenching factor for alpha particles vary in the range of (0.5-1.2) keV/MeV and (0.07-0.17), respectively, due to energy dependence of the emitted scintillating light in the energy interval (2.0-7.0) MeV. The integral luminescence intensity of the Li6Eu(BO3)(3) crystal increases by more than four times only at low temperatures, below 80 K. Therefore, the Li6Eu(BO3)(3)-based cryogenic scintillating bolometers can be attractive detectors for direct neutron flux monitoring, to search for rare alpha decays or solar axions.

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