Figure/Plot | Description | ||||||
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SABRE South simulated through GEANT4 | |||||||
SABRE South enclosure simulated through GEANT4 | |||||||
| The exclusion and discovery power of SABRE South for a DAMA/LIBRA-like signal. The shaded regions indicate 1 sigma statistical uncertainty bands. SABRE South is expected to reject the DAMA/LIBRA modulation at 3 sigma (in the case of null results) or confirm it at 5 sigma (in the event of observation of a compatible modulation) within 2.5 years. View file | | name | south_exclusion_curve.pdf||||
90% exclusion curve for the SABRE South experiment after 3 years of data taking assuming a background model in the 1–6 keVee and an exposure mass of 50 kg. The best fits to the DAMA/LIBRA data for this model in both the low and high-mass region are shown in pink. (Version from https://arxiv.org/pdf/2205.13849.pdf) | |||||||
| SABRE South total simulated background (Version from https://arxiv.org/pdf/2205.13849.pdf) | ||||||
| SABRE South Crystal Intrinsic | ||||||
| SABRE South Veto Comparison 40K | ||||||
| SABRE South Veto Comparison All | ||||||
| SABRE South Cosmogenic decay | ||||||
Background components and veto efficiency | |||||||
SABRE South full background simulations |
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