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| Home > Publications database > JUNO's sensitivity to 7Be, pep and CNO solar neutrinos and strategy for directional analysis of CNO solar neutrinos in JUNO > print |
| 001 | 338879 | ||
| 005 | 20230405003854.0 | ||
| 037 | _ | _ | |a GSI-2023-00520 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |a Singhal, Apeksha |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 86th Annual Conference of the DPG and DPG Spring Meeting |g SMuK23 |c Dresden |d 2023-03-20 - 2023-03-24 |w Germany |
| 245 | _ | _ | |a JUNO's sensitivity to 7Be, pep and CNO solar neutrinos and strategy for directional analysis of CNO solar neutrinos in JUNO |
| 260 | _ | _ | |c 2023 |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Other |2 DataCite |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a LECTURE_SPEECH |2 ORCID |
| 336 | 7 | _ | |a Conference Presentation |b conf |m conf |0 PUB:(DE-HGF)6 |s 1680594680_1976 |2 PUB:(DE-HGF) |x After Call |
| 520 | _ | _ | |a JUNO Experiment is 20 kt multipurpose LS detector, under construction in China, with planned completion in 2023. Its main goal is Neutrino Mass Ordering determination, exploiting its large target mass and excellent energy resolution (3% at 1 MeV). Due to its unique properties, JUNO will have potential of real-time solar neutrino measurement with unprecedented levels of precision using multivariate (MV) fit. Sensitivity study is performed by considering all possible sources of background, including their various concentration level and full simulation of detector response. Performing directional analysis of CNO solar neutrinos via Correlated and Integrated Directionality method (developed by Borexino collaboration) in JUNO and using it as additional constraint in MV fit has potential to further improve precision of CNO solar neutrino measurement. This talk will summarize methods for sensitivity studies using MV fit and the final results. Investigation of Cherenkov and scintillation light properties using JUNO MC software and strategies of preliminary directional analysis will be shown. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF4-612) |0 G:(DE-HGF)POF4-612 |c POF4-612 |f POF IV |x 0 |
| 700 | 1 | _ | |a Liu, Runxuan |0 P:(DE-Ds200)OR12410 |b 1 |
| 700 | 1 | _ | |a Ludhova, Livia |0 P:(DE-HGF)0 |b 2 |
| 700 | 1 | _ | |a Meraviglia, Anita |0 P:(DE-Ds200)OR11827 |b 3 |
| 700 | 1 | _ | |a Mohan, Nikhil |0 P:(DE-Ds200)OR11201 |b 4 |
| 700 | 1 | _ | |a Pelicci, Luca |0 P:(DE-HGF)0 |b 5 |
| 700 | 1 | _ | |a Rifai, Mariam |0 P:(DE-HGF)0 |b 6 |
| 700 | 1 | _ | |a Vollbrecht, Moritz Cornelius |0 P:(DE-Ds200)OR12429 |b 7 |
| 856 | 4 | _ | |u https://www.dpg-verhandlungen.de/year/2023/conference/smuk/part/t/session/13/contribution/3 |
| 909 | C | O | |o oai:repository.gsi.de:338879 |p VDB |
| 910 | 1 | _ | |a GSI Helmholtzzentrum für Schwerionenforschung GmbH |0 I:(DE-Ds200)20121206GSI |k GSI |b 3 |6 P:(DE-Ds200)OR11827 |
| 910 | 1 | _ | |a GSI Helmholtzzentrum für Schwerionenforschung GmbH |0 I:(DE-Ds200)20121206GSI |k GSI |b 4 |6 P:(DE-Ds200)OR11201 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-612 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2023 |
| 920 | _ | _ | |l yes |
| 920 | 1 | _ | |0 I:(DE-Ds200)FFN-20210302OR452 |k FFN |l FAIR Forschung NRW |x 0 |
| 980 | _ | _ | |a conf |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a I:(DE-Ds200)FFN-20210302OR452 |
| 980 | _ | _ | |a UNRESTRICTED |
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