Measurement of neutron-proton capture in the SNO+ water phase
Publikation: Beitrag in Fachzeitschrift › Forschungsartikel › Beigetragen › Begutachtung
Beitragende
- University of Sussex
- Laboratório de Instrumentação e Física Experimental de Partículas
- Universidade de Lisboa
- Norwich University
- Universidad Nacional Autónoma de México
- The University of Chicago
- Queen Mary University of London
- Lancaster University
- Laurentian University
- MTA Atomki, 4001 Debrecen, Hungary
- Boston University
- University of California at Berkeley
- King's College London (KCL)
- Technische Universität Dresden
- Lawrence Berkeley National Laboratory
- TRIUMF
- SNOLAB, Creighton Mine #9, 1039 Regional Road 24, Sudbury, Ontario P3Y 1N2, Canada
Abstract
The SNO + experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV γ 's produced by neutron capture on hydrogen were made using an Am-Be calibration source, for which a large fraction of emitted neutrons are produced simultaneously with a 4.4-MeV γ . Analysis of the delayed coincidence between the 4.4-MeV γ and the 2.2-MeV capture γ revealed a neutron detection efficiency that is centered around 50% and varies at the level of 1% across the inner region of the detector, which to our knowledge is the highest efficiency achieved among pure water Cherenkov detectors. In addition, the neutron capture time constant was measured and converted to a thermal neutron-proton capture cross section of 336 .3-1.5+1.2mb .
Details
Originalsprache | Englisch |
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Seiten (von - bis) | 14002 |
Fachzeitschrift | Physical Review C, Nuclear physics |
Jahrgang | 102 |
Ausgabenummer | 1 |
Publikationsstatus | Veröffentlicht - 1 Juli 2020 |
Peer-Review-Status | Ja |
Externe IDs
Scopus | 85092928789 |
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BibCode | 2020PhRvC.102a4002A |
ORCID | /0000-0001-7323-7816/work/142257373 |
Schlagworte
Schlagwörter
- Neutrinos, Solare neutrinos, Sudbury Neutrino Obs. SNO