Journal article
Cosmic ray background rejection with wire-cell LArTPC event reconstruction in the MicroBooNE detector
- Abstract:
- For a large liquid-argon time-projection chamber (LArTPC) operating on or near the Earth's surface to detect neutrino interactions, the rejection of cosmogenic background is a critical and challenging task because of the large cosmic-ray flux and the long drift time of the time-projection chamber. We introduce a superior cosmic background rejection procedure based on the Wire-Cell three-dimensional (3D) event reconstruction for LArTPCs. From an initial 1:20 000 neutrino to cosmic-ray background ratio, we demonstrate these tools on data from the MicroBooNE experiment and create a high-performance generic neutrino event selection with a cosmic contamination of 14.9% (9.7%) for a visible energy region greater than O(200) MeV. The neutrino interaction selection efficiency is 80.4% and 87.6% for inclusive νμ charged-current and νe charged-current interactions, respectively. This significantly improved performance compared with existing reconstruction algorithms marks a major milestone toward reaching the scientific goals of LArTPC neutrino oscillation experiments operating near the Earth's surface.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
-
-
(Preview, Accepted manuscript, 7.0MB, Terms of use)
-
- Publisher copy:
- 10.1103/PhysRevApplied.15.064071
- Publisher:
- American Physical Society
- Journal:
- Physical Review Applied More from this journal
- Volume:
- 15
- Issue:
- 6
- Article number:
- 64071
- Publication date:
- 2021-06-29
- Acceptance date:
- 2021-03-26
- DOI:
- EISSN:
-
2331-7019
- ISSN:
-
2331-7019
- Language:
-
English
- Keywords:
- Pubs id:
-
1185766
- Local pid:
-
pubs:1185766
- Deposit date:
-
2022-01-11
Terms of use
- Copyright holder:
- American Physical Society
- Copyright date:
- 2021
- Rights statement:
- © 2021 American Physical Society
- Notes:
- This is the accepted manuscript version of the article. The final version is available online from American Physical Society at: https://doi.org/10.1103/PhysRevApplied.15.064071
If you are the owner of this record, you can report an update to it here: Report update to this record