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Sensitivity to neutrino-antineutrino transitions for boron neutrinos - MaRDI portal

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Sensitivity to neutrino-antineutrino transitions for boron neutrinos

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Publication:2295519

DOI10.1016/J.NUCLPHYSB.2019.114661zbMATH Open1430.81093arXiv1905.05464OpenAlexW2946486567WikidataQ127761510 ScholiaQ127761510MaRDI QIDQ2295519

Author name not available (Why is that?)

Publication date: 13 February 2020

Published in: (Search for Journal in Brave)

Abstract: Neutrino-antineutrino conversion is an important new physics process. The observation of this phenomenon could indicate total lepton number violation and potential CPT-violation. Searching for the appearance of electron antineutrinos from solar neutrinos from m8B decay allows us to hunt for this rare process, although it can also be explained by other mechanisms or hypotheses. This analysis examines the capabilities of observing neutrino-antineutrino transition from m8B unoscillated solar neutrinos using different liquid scintillator detector configurations. High energy reactor neutrinos and atmospheric neutrinos are the two dominant background sources. Large volume liquid scintillator detectors with deep underground shielding, placed far away from reactors and with capabilities of pulse shaped discrimination will significantly increase the search sensitivity. It is demonstrated that for the next generation of large liquid scintillator detectors being planned or under construction, the sensitivity to the average probability of neutrino-antineutrino transitions can reach 10−6, which is an order of magnitude better than the current best experimental limits.


Full work available at URL: https://arxiv.org/abs/1905.05464




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