Figure/Plot | Description |
|---|---|
 | Collection of observed modulation rates by NaI experiments (+global average) as of the end of 2021. |
 | Similar to above, but the DAMA observation is replaced with the modulation expected for the DM model given in the figure for a range of QFs. Purpose is to demonstrate how much an observation might change given different crystal dependent quenching factors. |
 | Labelled version of the SABRE South render |
 | SABRE South rendering |
 | 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 years. | |
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. |
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