期刊
JOURNAL OF HIGH ENERGY PHYSICS
卷 -, 期 6, 页码 -出版社
SPRINGER
DOI: 10.1007/JHEP06(2022)062
关键词
Neutrino Detectors and Telescopes (experiments)
资金
- Chinese Academy of Sciences
- National Key R&D Program of China
- CAS Center for Excellence in Particle Physics, Wuyi University
- Tsung-Dao Lee Institute of Shanghai Jiao Tong University in China
- Institut National de Physique Nucleaire et de Physique des Particulest (IN2P3) in France
- Istituto Nazionale di Fisica Nucleare (INFN) in Italy
- Italian-Chinese collaborative research program MAECI-NSFC
- Fond de la Recherche Scientifique (F.R.S-FNRS)
- FWO under the Excellence of Science -EOS in Belgium
- Conselho Nacional de Desenvolvimento Cientifico e Tecnologico in Brazil
- Agencia Nacional de Investigacion y Desarrollo in Chile
- Charles University Research Centre
- Ministry of Education, Youth, and Sports in Czech Republic
- Deutsche Forschungsgemeinschaft (DFG)
- Helmholtz Association
- Cluster of Excellence PRISMA+ in Germany
- Joint Institute of Nuclear Research (JINR)
- Lomonosov Moscow State University in Russia
- joint Russian Science Foundation (RSF)
- National Natural Science Foundation of China (NSFC) research program
- MOST in Taiwan
- MOE in Taiwan
- Chulalongkorn University
- Suranaree University of Technology in Thailand
- University of California at Irvine in U.S.A
This study focuses on the investigation of damping signatures at the Jiangmen Underground Neutrino Observatory (JUNO), including various new physics models such as quantum decoherence, nu(3) decay, neutrino absorption, and wave packet decoherence. The findings suggest that JUNO can significantly improve the limits on these damping parameters compared to current experimental limits, as well as distinguish the different damping signatures in practical experiments.
We study damping signatures at the Jiangmen Underground Neutrino Observatory (JUNO), a medium-baseline reactor neutrino oscillation experiment. These damping signatures are motivated by various new physics models, including quantum decoherence, nu(3) decay, neutrino absorption, and wave packet decoherence. The phenomenological effects of these models can be characterized by exponential damping factors at the probability level. We assess how well JUNO can constrain these damping parameters and how to disentangle these different damping signatures at JUNO. Compared to current experimental limits, JUNO can significantly improve the limits on tau(3)/m(3) in the nu(3) decay model, the width of the neutrino wave packet sigma(x), and the intrinsic relative dispersion of neutrino momentum sigma(rel).
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