- Background Norm
- Non linearity
- [](##Cherenkov contribution)
- [](##Energy Scale)
- [](##Energy Resolution)
- [](##Energy Loss)
- [](##Background Scaling)
- [](##Segment to Segment Volume)
- [](##Segment to Segment efficiency)
- [](##Segment to Segment energy Scale)
- [](##Segment to Segment energy resolution)
- [](##Segment to Segment energy loss)
- [](##Baseline Uncertainty)
- [](##Al-28 activation spectrum)
- [](##Non-eq contribution)
- [](##nH peak)
- [](##Segment to Segment nH peak)
- [](##Wall thickness)
- [](##Z fiducial cut)
- [](##Energy Threshold)
- [](##Segment to Segment Energy Threshold)
- Energy Smearing
The biggest variation from atmospheric pressure variation is 1%. If we conservatively estimate a 100% uncertaintiy on this estimate, there will be a 1% background norm uncertainty. Study by XIangpan shows that there is no variation in sensitivity when 10% is used.
make generateLvsEELossCovMatrix
./generateLvsEELossCovMatrix test_6.root LvsEELossCovMatrix.root 0.008 1000
Al - 27 in the core in the reaction, then will activated capturing neutron be converted to Al-28 then will produce beta decay (will produce antineutrino ) 2.86 MeV
neutron capture in hidrogen 2.22MeV gamma (big background)