Abstract
Cosmogenic isotopes 9Li and 8He produced in the detector are the most problematic background in the reactor neutrino experiments designed to determine precisely the neutrino mixing angle θ13. The average time interval of cosmic-ray muons in the detector is often on the order of the lifetimes of the 9Li and 8He isotopes. We have developed a method for determining this kind of background from the distribution of time since last muon for muon rate up to about 20 Hz when the background-to-signal ratio is small, on the order of a few percents.
| Original language | English |
|---|---|
| Pages (from-to) | 471-474 |
| Number of pages | 4 |
| Journal | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
| Volume | 564 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Aug 2006 |
| Externally published | Yes |
Keywords
- Li
- Neutrino oscillation
- Reactor
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