Review Article
Current Status and Future Prospects of the SNO+ Experiment
Table 2
Target levels, in g/g, and corresponding decay rates for the internal 238U- and 232Th-chain contaminants in the various SNO+ phases. Secular equilibrium has been assumed for all the isotopes except 210Pb, 210Bi, and 210Po. The levels of 210Bi and 210Po during the pure scintillator phase and the Te-loaded phase are expected to be out of secular equilibrium due to the intrinsic scintillator contamination and the leaching off of the AV surface. For the 0.3% Te-loaded scintillator the tellurium/polonium affinity component is also included in the 210Po decays/yr (see text).
| |||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Expected number of events in the first year after 9 months of water phase. Expected number of events in the first year after 9 months of water phase followed by 6 months of pure scintillator phase. |