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- W4312127588 abstract "Abstract We present here the model dependent and independent sensitivity studies for NaI detectors designed to test the DAMA result, and compare the predicted limits from SABRE with the present performance of both ANAIS and COSINE. We find that the strongest discovery and exclusion limits are set by a detector with the lowest background (assuming equal live times), and also note that our method correctly computes the present exclusion limits previously published by ANAIS and COSINE. In particular, with a target mass of 50 kg and background rate of 0.36 cpd/kg/keV (after veto), SABRE will be able to exclude the DAMA signal with 3 $$sigma $$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mi>σ</mml:mi> </mml:math> confidence or ‘discover’ it with 5 $$sigma $$ <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML> <mml:mi>σ</mml:mi> </mml:math> confidence within 2 years. This strongly motivates the quest for ever lower backgrounds in NaI detectors." @default.
- W4312127588 created "2023-01-04" @default.
- W4312127588 creator A5018851183 @default.
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- W4312127588 date "2022-12-12" @default.
- W4312127588 modified "2023-10-18" @default.
- W4312127588 title "Influence of NaI background and mass on testing the DAMA modulation" @default.
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- W4312127588 doi "https://doi.org/10.1140/epjc/s10052-022-11062-w" @default.
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