Understanding internal backgrounds of NaI(Tl) crystals toward a 200~kg array for the KIMS-NaI experiment
P. Adhikari, G. Adhikari, S. Choi, C. Ha, I.S. Hahn, E.J. Jeon, H.W., Joo, W.G. Kang, H.J. Kim, H.O. Kim, K.W. Kim, N.Y. Kim, S.K. Kim, Y.D. Kim,, Y.H. Kim, H.S. Lee, J.H. Lee, M.H. Lee, D.S. Leonard, J. Li, S.Y. Oh, S.L., Olsen, H.K. Park, H.S. Park, K.S. Park, J.H. So

TL;DR
This paper discusses the development and characterization of low-background NaI(Tl) crystals for the KIMS-NaI dark matter detection experiment, aiming to test DAMA/LIBRA's annual modulation signal.
Contribution
It presents new measurements of internal radioisotope contamination in prototype crystals and estimates the background reduction achievable for a 200 kg detector array.
Findings
Progress in reducing internal contaminations of radioisotopes.
Expected background level below 1 count/day/keV/kg near 2 keV.
Potential for a 7σ unambiguous test of DAMA/LIBRA's signature with 600 kg·year exposure.
Abstract
The Korea Invisible Mass Search (KIMS) collaboration has developed low-background NaI(Tl) crystals that are suitable for the direct detection of WIMP dark matter. With experience built on the KIMS-CsI programs, the KIMS-NaI experiment will consist of a 200~kg NaI(Tl) crystal array surrounded by layers of shielding structures and will be operated at the Yangyang underground laboratory. The goal is to provide an unambiguous test of the DAMA/LIBRA's annual modulation signature. Measurements of six prototype crystals show progress in the reduction of internal contaminations of radioisotopes. Based on our understanding of these measurements, we expect to achieve a background level in the final detector configuration that is less than 1~count/day/keV/kg for recoil energies around 2~keV. The annual modulation sensitivity for the KIMS-NaI experiment shows that an unambiguous 7 test of…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle Detector Development and Performance · Astrophysics and Cosmic Phenomena
