guest ::
| Home > Publications database > JUNO Non-oscillation Physics > print |
| Home > Publications database > JUNO Non-oscillation Physics > print |
| 001 | 906366 | ||
| 005 | 20251027132711.0 | ||
| 024 | 7 | _ | |a 10.1088/1742-6596/2156/1/012109 |2 doi |
| 024 | 7 | _ | |a 1742-6588 |2 ISSN |
| 024 | 7 | _ | |a 1742-6596 |2 ISSN |
| 024 | 7 | _ | |a 2128/30765 |2 Handle |
| 024 | 7 | _ | |a WOS:001432940800109 |2 WOS |
| 037 | _ | _ | |a FZJ-2022-01395 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Settanta, Giulio |0 P:(DE-Juel1)180506 |b 0 |e Corresponding author |u fzj |
| 111 | 2 | _ | |a 17th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2021) |g TAUP 2021 |c Online (Valencia) |d 2021-08-30 - 2021-09-03 |w Spain |
| 245 | _ | _ | |a JUNO Non-oscillation Physics |
| 260 | _ | _ | |a Bristol |c 2021 |b IOP Publ. |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2021-12-01 |
| 264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2021-12-01 |
| 300 | _ | _ | |a 2156 012109 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |m journal |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1645538014_20024 |2 PUB:(DE-HGF) |
| 520 | _ | _ | |a The 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. |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF4-612) |0 G:(DE-HGF)POF4-612 |c POF4-612 |f POF IV |x 0 |
| 542 | _ | _ | |i 2021-12-01 |2 Crossref |u http://creativecommons.org/licenses/by/3.0/ |
| 542 | _ | _ | |i 2021-12-01 |2 Crossref |u https://iopscience.iop.org/info/page/text-and-data-mining |
| 588 | _ | _ | |a Dataset connected to CrossRef, Journals: juser.fz-juelich.de |
| 773 | 1 | 8 | |a 10.1088/1742-6596/2156/1/012109 |b IOP Publishing |d 2021-12-01 |n 1 |p 012109 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 773 | _ | _ | |a 10.1088/1742-6596/2156/1/012109 |g Vol. 2156, no. 1, p. 012109 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012109 |t Journal of physics / Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/906366/files/Settanta_2021_J._Phys.__Conf._Ser._2156_012109.pdf |y OpenAccess |
| 909 | C | O | |o oai:juser.fz-juelich.de:906366 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a Forschungszentrum Jülich |0 I:(DE-588b)5008462-8 |k FZJ |b 0 |6 P:(DE-Juel1)180506 |
| 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 2022 |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 3.0 |0 LIC:(DE-HGF)CCBY3 |2 HGFVOC |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0200 |2 StatID |b SCOPUS |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0300 |2 StatID |b Medline |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 920 | _ | _ | |l yes |
| 920 | 1 | _ | |0 I:(DE-Juel1)IKP-2-20111104 |k IKP-2 |l Experimentelle Hadrondynamik |x 0 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a I:(DE-Juel1)IKP-2-20111104 |
| 980 | 1 | _ | |a FullTexts |
| 999 | C | 5 | |1 Adam |y 2015 |2 Crossref |o Adam 2015 |
| 999 | C | 5 | |1 Abusleme |y 2021 |2 Crossref |o Abusleme 2021 |
| 999 | C | 5 | |a 10.1088/0954-3899/43/3/030401 |1 An |9 -- missing cx lookup -- |2 Crossref |t J. Phys. G: Nucl. Part. Phys. |v 43 |y 2016 |
| 999 | C | 5 | |1 Li |y 2020 |2 Crossref |o Li 2020 |
| 999 | C | 5 | |a 10.1088/1674-1137/abd92a |1 Abusleme |9 -- missing cx lookup -- |2 Crossref |t Chin. phys. C |v 45 |y 2021 |
| 999 | C | 5 | |1 Settanta |y 2019 |2 Crossref |o Settanta 2019 |
| 999 | C | 5 | |a 10.1140/epjc/s10052-021-09565-z |9 -- missing cx lookup -- |1 Abusleme |p 887 - |2 Crossref |t Eur. Phys. C |v 81 |y 2021 |
| 999 | C | 5 | |a 10.1103/PhysRevD.92.023004 |1 Honda |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. D |v 92 |y 2015 |
| 999 | C | 5 | |a 10.1103/PhysRevD.94.052001 |1 Richard |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. D |v 94 |y 2016 |
| 999 | C | 5 | |a 10.1007/BF01556368 |9 -- missing cx lookup -- |1 Daum |p 417 - |2 Crossref |t Zeit. fur Phys. C Part, and Fields |v 66 |y 1995 |
| 999 | C | 5 | |a 10.1029/2018JB016681 |9 -- missing cx lookup -- |1 Reguzzoni |p 4231 - |2 Crossref |t Journ. of Geophys. Res.: Solid Earth |v 124 |y 2019 |
| 999 | C | 5 | |1 Ruohan |y 2020 |2 Crossref |o Ruohan 2020 |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|