000906369 001__ 906369
000906369 005__ 20230217124542.0
000906369 0247_ $$2doi$$a10.1088/1742-6596/2156/1/012202
000906369 0247_ $$2ISSN$$a1742-6588
000906369 0247_ $$2ISSN$$a1742-6596
000906369 0247_ $$2Handle$$a2128/30761
000906369 037__ $$aFZJ-2022-01398
000906369 082__ $$a530
000906369 1001_ $$0P:(DE-Juel1)180507$$aSinghal, Apeksha$$b0$$eCorresponding author
000906369 1112_ $$a17th International Conference on Topics in Astroparticle and Underground Physics$$cValencia (online)$$d2021-08-26 - 2021-09-03$$gTAUP 2021$$wSpain
000906369 245__ $$aUnderstanding the systematic effects for the directional detection of sub-MeV solar neutrinos with Borexino
000906369 260__ $$aBristol$$bIOP Publ.$$c2021
000906369 264_1 $$2Crossref$$3print$$bIOP Publishing$$c2021-12-01
000906369 264_1 $$2Crossref$$3print$$bIOP Publishing$$c2021-12-01
000906369 300__ $$a5
000906369 3367_ $$2ORCID$$aCONFERENCE_PAPER
000906369 3367_ $$033$$2EndNote$$aConference Paper
000906369 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000906369 3367_ $$2BibTeX$$aINPROCEEDINGS
000906369 3367_ $$2DRIVER$$aconferenceObject
000906369 3367_ $$2DataCite$$aOutput Types/Conference Paper
000906369 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1645533868_26051
000906369 520__ $$aBorexino, located at the Laboratori Nazionali del Gran Sasso in Italy, is a liquid scintillator detector that measures solar neutrinos via elastic scattering off electrons. The scintillation process of detection makes it impossible to distinguish electrons scattered by neutrinos from the electrons emitted from the decays of radioactive backgrounds. Due to the unprecedented radio-purity achieved by the Borexino detector, the real time spectroscopic detection of solar neutrinos from both the pp chain and CNO fusion cycle of the Sun has been performed. With the newly presented analysis, it is now possible for the first time, to perform the directional detection of the sub-MeV solar neutrinos and extract the 7Be interaction rate using the few Cherenkov photons emitted at early times, in the direction of scattered electrons with an energy threshold of 0.16 MeV in the liquid scintillator. The angle which correlates the direction of the Sun and the direction of the emitted Cherenkov photons is a key parameter to extract the neutrino signal from data. This article will describe the strategy used in the evaluation of various systematic effects including the geometric conditions of the detector and the data selection cuts that can influence the shape of the directional angle distribution for backgrounds, which is crucial to disentangle the directional sub-MeV solar neutrino signal from the isotropic background in data.
000906369 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000906369 542__ $$2Crossref$$i2021-12-01$$uhttp://creativecommons.org/licenses/by/3.0/
000906369 542__ $$2Crossref$$i2021-12-01$$uhttps://iopscience.iop.org/info/page/text-and-data-mining
000906369 588__ $$aDataset connected to CrossRef, Journals: juser.fz-juelich.de
000906369 77318 $$2Crossref$$3journal-article$$a10.1088/1742-6596/2156/1/012202$$bIOP Publishing$$d2021-12-01$$n1$$p012202$$tJournal of Physics: Conference Series$$v2156$$x1742-6588$$y2021
000906369 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/2156/1/012202$$gVol. 2156, no. 1, p. 012202 -$$n1$$p012202$$tJournal of physics / Conference Series$$v2156$$x1742-6588$$y2021
000906369 8564_ $$uhttps://juser.fz-juelich.de/record/906369/files/Understanding%20the%20systematic%20effects%20for%20the%20directional%20detection%20of%20sub-MeV%20solar%20neutrinos%20with%20Borexino.pdf$$yOpenAccess
000906369 909CO $$ooai:juser.fz-juelich.de:906369$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000906369 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)180507$$aForschungszentrum Jülich$$b0$$kFZJ
000906369 9131_ $$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$$x0
000906369 9141_ $$y2022
000906369 915__ $$0LIC:(DE-HGF)CCBY3$$2HGFVOC$$aCreative Commons Attribution CC BY 3.0
000906369 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000906369 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000906369 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000906369 920__ $$lyes
000906369 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
000906369 980__ $$acontrib
000906369 980__ $$aVDB
000906369 980__ $$aUNRESTRICTED
000906369 980__ $$ajournal
000906369 980__ $$aI:(DE-Juel1)IKP-2-20111104
000906369 9801_ $$aFullTexts
000906369 999C5 $$1Agostini$$2Crossref$$oAgostini 2021$$y2021
000906369 999C5 $$1Agostini$$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.100.082004$$tPhys. Rev. D$$v100$$y2019
000906369 999C5 $$1Martyn$$2Crossref$$oMartyn 2021$$y2021
000906369 999C5 $$1Kumaran$$2Crossref$$oKumaran 2021$$y2021