Tau Neutrino Appearance in the Flux of Atmospheric Neutrinos
2023.04.24 16:13 - Katarzyna KuźniarSeria:
Seminarium doktoranckie
Prelegent i afiliacja:
Maitrayee Mandal (Szkoła Doktorska NCBJ)
Data:
czw., 2023-04-27 09:15 do 10:15
Miejsce:
room 207, Pasteura 7 / https://www.gotomeet.me/NCBJmeetings/phd-seminar / https://events.ncbj.gov.pl/e/PhDSeminar2223
Streszczenie:
The flux of atmospheric neutrinos comprises of muon and electron neutrinos. Below 10 GeV, we do not expect to see a significant number of tau neutrinos in the atmosphere, unless they appear from the oscillation of atmospheric muon neutrinos. The Super-Kamiokande experiment (Super-K) is a water Cherenkov detector in Japan. Super-K is capable of directly detecting these oscillated tau neutrinos - which would be an unambiguous confirmation of the phenomena of neutrino oscillations. The last study at Super-K, in 2018, excluded the hypothesis of no tau neutrino appearance at 4.6 sigma. This seminar presents the latest analysis on the subject.
Załączniki:
Załącznik | Wielkość |
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seminarium_studium_doktoranckiego_ncbj_27-04-2023.docx | 13.05 KB |
seminarium_studium_doktoranckiego_ncbj_27-04-2023.pdf | 303.91 KB |