000338879 001__ 338879
000338879 005__ 20230405003854.0
000338879 037__ $$aGSI-2023-00520
000338879 041__ $$aEnglish
000338879 1001_ $$0P:(DE-HGF)0$$aSinghal, Apeksha$$b0$$eCorresponding author
000338879 1112_ $$a86th Annual Conference of the DPG and DPG Spring Meeting$$cDresden$$d2023-03-20 - 2023-03-24$$gSMuK23$$wGermany
000338879 245__ $$aJUNO's sensitivity to 7Be, pep and CNO solar neutrinos and strategy for directional analysis of CNO solar neutrinos in JUNO
000338879 260__ $$c2023
000338879 3367_ $$033$$2EndNote$$aConference Paper
000338879 3367_ $$2DataCite$$aOther
000338879 3367_ $$2BibTeX$$aINPROCEEDINGS
000338879 3367_ $$2DRIVER$$aconferenceObject
000338879 3367_ $$2ORCID$$aLECTURE_SPEECH
000338879 3367_ $$0PUB:(DE-HGF)6$$2PUB:(DE-HGF)$$aConference Presentation$$bconf$$mconf$$s1680594680_1976$$xAfter Call
000338879 520__ $$aJUNO 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.
000338879 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000338879 7001_ $$0P:(DE-Ds200)OR12410$$aLiu, Runxuan$$b1
000338879 7001_ $$0P:(DE-HGF)0$$aLudhova, Livia$$b2
000338879 7001_ $$0P:(DE-Ds200)OR11827$$aMeraviglia, Anita$$b3
000338879 7001_ $$0P:(DE-Ds200)OR11201$$aMohan, Nikhil$$b4
000338879 7001_ $$0P:(DE-HGF)0$$aPelicci, Luca$$b5
000338879 7001_ $$0P:(DE-HGF)0$$aRifai, Mariam$$b6
000338879 7001_ $$0P:(DE-Ds200)OR12429$$aVollbrecht, Moritz Cornelius$$b7
000338879 8564_ $$uhttps://www.dpg-verhandlungen.de/year/2023/conference/smuk/part/t/session/13/contribution/3
000338879 909CO $$ooai:repository.gsi.de:338879$$pVDB
000338879 9101_ $$0I:(DE-Ds200)20121206GSI$$6P:(DE-Ds200)OR11827$$aGSI Helmholtzzentrum für Schwerionenforschung GmbH$$b3$$kGSI
000338879 9101_ $$0I:(DE-Ds200)20121206GSI$$6P:(DE-Ds200)OR11201$$aGSI Helmholtzzentrum für Schwerionenforschung GmbH$$b4$$kGSI
000338879 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
000338879 9141_ $$y2023
000338879 920__ $$lyes
000338879 9201_ $$0I:(DE-Ds200)FFN-20210302OR452$$kFFN$$lFAIR Forschung NRW$$x0
000338879 980__ $$aconf
000338879 980__ $$aVDB
000338879 980__ $$aI:(DE-Ds200)FFN-20210302OR452
000338879 980__ $$aUNRESTRICTED