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9 results on '"Aiello, Sebastiano"'

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1. Feasibility and physics potential of detecting 8B solar neutrinos at JUNO * *This work was supported by the Chinese Academy of Sciences, the National Key R&D Program of China, the CAS Center for Excellence in Particle Physics, the Joint Large-Scale Scientific Facility Funds of the NSFC and CAS, Wuyi University, and the Tsung-Dao Lee Institute of Shanghai Jiao Tong University in China, the Institut National de Physique Nucléaire et de Physique de Particules (IN2P3) in France, the Istituto Nazionale di Fisica Nucleare (INFN) in Italy, the Fond de la Recherche Scientifique (F.R.S-FNRS) and FWO under the “Excellence of Science – EOS” in Belgium, the Conselho Nacional de Desenvolvimento Científico e Tecnològico in Brazil, the Agencia Nacional de Investigación y Desarrollo in Chile, the Charles University Research Centre and the Ministry of Education, Youth, and Sports in Czech Republic, the Deutsche Forschungsgemeinschaft (DFG), the Helmholtz Association, and the Cluster of Excellence PRISMA+ in Germany, the

2. JUNO Physics Prospects

3. JUNO sensitivity to low energy atmospheric neutrino spectra

4. Sub-percent precision measurement of neutrino oscillation parameters with JUNO*\t\t\t\t *Supported by the Chinese Academy of Sciences, the National Key R&D Program of China, the CAS Center for Excellence in Particle Physics, Wuyi University, and the Tsung-Dao Lee Institute of Shanghai Jiao Tong University in China, the Institut National de Physique Nucléaire et de Physique de Particules (IN2P3) in France, the Istituto Nazionale di Fisica Nucleare (INFN) in Italy, the Italian-Chinese collaborative research program MAECI-NSFC, the Fond de la Recherche Scientifique (F.R.S-FNRS) and FWO under the

5. Damping signatures at JUNO, a medium-baseline reactor neutrino oscillation experiment.

6. JUNO sensitivity to low energy atmospheric neutrino spectra.

7. Sub-percent Precision Measurement of Neutrino Oscillation Parameters with JUNO

8. Sub-percent precision measurement of neutrino oscillation parameters with JUNO

9. KM3NeT Detection Unit Line Fit reconstruction using positioning sensors data

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