Improved measurement of 8B solar neutrinos with 1.5 kt· y of Borexino exposure
Research output: Contribution to journal › Research article › Contributed › peer-review
Contributors
- Technical University of Munich
- University of Milan
- Princeton University
- University of Hamburg
- Virginia Polytechnic Institute and State University
- Lomonosov Moscow State University
- Institute for Celestial Mechanics and Computation of Ephemerides
- University of Tübingen
- Johannes Gutenberg University Mainz
- University of Houston
- Jagiellonian University in Kraków
- NASU - Institute of Nuclear Research
- RWTH Aachen University
- Moscow Engineering Physics Institute
Abstract
We report on an improved measurement of the B8 solar neutrino interaction rate with the Borexino experiment at the Laboratori Nazionali del Gran Sasso. Neutrinos are detected via their elastic scattering on electrons in a large volume of liquid scintillator. The measured rate of scattered electrons above 3 MeV of energy is 0.223-0.016+0.015(stat) -0.006+0.006(syst) cpd/100 t, which corresponds to an observed solar neutrino flux assuming no neutrino flavor conversion of φB8ES=2.57-0.18+0.17(stat) -0.07+0.07(syst)×106 cm-2 s-1. This measurement exploits the active volume of the detector in almost its entirety for the first time, and takes advantage of a reduced radioactive background following the 2011 scintillator purification campaign and of novel analysis tools providing a more precise modeling of the background. Additionally, we set a new limit on the interaction rate of solar hep neutrinos, searched via their elastic scattering on electrons as well as their neutral current-mediated inelastic scattering on carbon, C12(ν,ν′)C∗12 (Eγ=15.1 MeV).
Details
Original language | English |
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Article number | 062001 |
Pages (from-to) | 1-14 |
Number of pages | 14 |
Journal | Physical review d |
Volume | 101 |
Issue number | 6 |
Publication status | Published - 15 Mar 2020 |
Peer-reviewed | Yes |