000906366 001__ 906366
000906366 005__ 20230217124541.0
000906366 0247_ $$2doi$$a10.1088/1742-6596/2156/1/012109
000906366 0247_ $$2ISSN$$a1742-6588
000906366 0247_ $$2ISSN$$a1742-6596
000906366 0247_ $$2Handle$$a2128/30765
000906366 037__ $$aFZJ-2022-01395
000906366 041__ $$aEnglish
000906366 082__ $$a530
000906366 1001_ $$0P:(DE-Juel1)180506$$aSettanta, Giulio$$b0$$eCorresponding author$$ufzj
000906366 1112_ $$a17th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2021)$$cOnline (Valencia)$$d2021-08-30 - 2021-09-03$$gTAUP 2021$$wSpain
000906366 245__ $$aJUNO Non-oscillation Physics
000906366 260__ $$aBristol$$bIOP Publ.$$c2021
000906366 264_1 $$2Crossref$$3print$$bIOP Publishing$$c2021-12-01
000906366 264_1 $$2Crossref$$3print$$bIOP Publishing$$c2021-12-01
000906366 300__ $$a2156 012109
000906366 3367_ $$2ORCID$$aCONFERENCE_PAPER
000906366 3367_ $$033$$2EndNote$$aConference Paper
000906366 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$mjournal
000906366 3367_ $$2BibTeX$$aINPROCEEDINGS
000906366 3367_ $$2DRIVER$$aconferenceObject
000906366 3367_ $$2DataCite$$aOutput Types/Conference Paper
000906366 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1645538014_20024
000906366 520__ $$aThe JUNO observatory, a 20 kt liquid scintillator detector to be completed in 2021 in China, belongs to the next-generation of neutrino detectors, which share the common features of having a multi-ton scale and an energy resolution at unprecedented levels. Beside the ambitious goal of neutrino mass ordering determination, the JUNO Collaboration plans also to perform a wide series of other measurements in the neutrino and astroparticle fields, rare processes and searches for new physics. The detector characteristics will allow the detection of neutrinos from many sources, like supernovae, the Sun, atmospheric and geoneutrinos. Other potential studies accessible to JUNO include the search for exotic processes, such as nucleon decays, Dark Matter and magnetic monopoles interactions, light sterile neutrinos production. This work reviews the physics potential of JUNO about non-reactor neutrino sources, highlighting the unique contributions that the experiment will give to the various fields in the forthcoming years.
000906366 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000906366 542__ $$2Crossref$$i2021-12-01$$uhttp://creativecommons.org/licenses/by/3.0/
000906366 542__ $$2Crossref$$i2021-12-01$$uhttps://iopscience.iop.org/info/page/text-and-data-mining
000906366 588__ $$aDataset connected to CrossRef, Journals: juser.fz-juelich.de
000906366 77318 $$2Crossref$$3journal-article$$a10.1088/1742-6596/2156/1/012109$$bIOP Publishing$$d2021-12-01$$n1$$p012109$$tJournal of Physics: Conference Series$$v2156$$x1742-6588$$y2021
000906366 773__ $$0PERI:(DE-600)2166409-2$$a10.1088/1742-6596/2156/1/012109$$gVol. 2156, no. 1, p. 012109 -$$n1$$p012109$$tJournal of physics / Conference Series$$v2156$$x1742-6588$$y2021
000906366 8564_ $$uhttps://juser.fz-juelich.de/record/906366/files/Settanta_2021_J._Phys.__Conf._Ser._2156_012109.pdf$$yOpenAccess
000906366 909CO $$ooai:juser.fz-juelich.de:906366$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000906366 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)180506$$aForschungszentrum Jülich$$b0$$kFZJ
000906366 9131_ $$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$$x0
000906366 9141_ $$y2022
000906366 915__ $$0LIC:(DE-HGF)CCBY3$$2HGFVOC$$aCreative Commons Attribution CC BY 3.0
000906366 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS
000906366 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline
000906366 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000906366 920__ $$lyes
000906366 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
000906366 980__ $$acontrib
000906366 980__ $$aVDB
000906366 980__ $$aUNRESTRICTED
000906366 980__ $$ajournal
000906366 980__ $$aI:(DE-Juel1)IKP-2-20111104
000906366 9801_ $$aFullTexts
000906366 999C5 $$1Adam$$2Crossref$$oAdam 2015$$y2015
000906366 999C5 $$1Abusleme$$2Crossref$$oAbusleme 2021$$y2021
000906366 999C5 $$1An$$2Crossref$$9-- missing cx lookup --$$a10.1088/0954-3899/43/3/030401$$tJ. Phys. G: Nucl. Part. Phys.$$v43$$y2016
000906366 999C5 $$1Li$$2Crossref$$oLi 2020$$y2020
000906366 999C5 $$1Abusleme$$2Crossref$$9-- missing cx lookup --$$a10.1088/1674-1137/abd92a$$tChin. phys. C$$v45$$y2021
000906366 999C5 $$1Settanta$$2Crossref$$oSettanta 2019$$y2019
000906366 999C5 $$1Abusleme$$2Crossref$$9-- missing cx lookup --$$a10.1140/epjc/s10052-021-09565-z$$p887 -$$tEur. Phys. C$$v81$$y2021
000906366 999C5 $$1Honda$$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.92.023004$$tPhys. Rev. D$$v92$$y2015
000906366 999C5 $$1Richard$$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.94.052001$$tPhys. Rev. D$$v94$$y2016
000906366 999C5 $$1Daum$$2Crossref$$9-- missing cx lookup --$$a10.1007/BF01556368$$p417 -$$tZeit. fur Phys. C Part, and Fields$$v66$$y1995
000906366 999C5 $$1Reguzzoni$$2Crossref$$9-- missing cx lookup --$$a10.1029/2018JB016681$$p4231 -$$tJourn. of Geophys. Res.: Solid Earth$$v124$$y2019
000906366 999C5 $$1Ruohan$$2Crossref$$oRuohan 2020$$y2020