Gast ::
| Hauptseite > Publikationsdatenbank > Understanding the systematic effects for the directional detection of sub-MeV solar neutrinos with Borexino > print |
| Hauptseite > Publikationsdatenbank > Understanding the systematic effects for the directional detection of sub-MeV solar neutrinos with Borexino > print |
| 001 | 906369 | ||
| 005 | 20230217124542.0 | ||
| 024 | 7 | _ | |a 10.1088/1742-6596/2156/1/012202 |2 doi |
| 024 | 7 | _ | |a 1742-6588 |2 ISSN |
| 024 | 7 | _ | |a 1742-6596 |2 ISSN |
| 024 | 7 | _ | |a 2128/30761 |2 Handle |
| 037 | _ | _ | |a FZJ-2022-01398 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a Singhal, Apeksha |0 P:(DE-Juel1)180507 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 17th International Conference on Topics in Astroparticle and Underground Physics |g TAUP 2021 |c Valencia (online) |d 2021-08-26 - 2021-09-03 |w Spain |
| 245 | _ | _ | |a Understanding the systematic effects for the directional detection of sub-MeV solar neutrinos with Borexino |
| 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 5 |
| 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 1645533868_26051 |2 PUB:(DE-HGF) |
| 520 | _ | _ | |a Borexino, 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. |
| 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 10.1088/1742-6596/2156/1/012202 |b IOP Publishing |d 2021-12-01 |n 1 |p 012202 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 773 | _ | _ | |a 10.1088/1742-6596/2156/1/012202 |g Vol. 2156, no. 1, p. 012202 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012202 |t Journal of physics / Conference Series |v 2156 |y 2021 |x 1742-6588 |
| 856 | 4 | _ | |u https://juser.fz-juelich.de/record/906369/files/Understanding%20the%20systematic%20effects%20for%20the%20directional%20detection%20of%20sub-MeV%20solar%20neutrinos%20with%20Borexino.pdf |y OpenAccess |
| 909 | C | O | |o oai:juser.fz-juelich.de:906369 |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)180507 |
| 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 Agostini |y 2021 |2 Crossref |o Agostini 2021 |
| 999 | C | 5 | |a 10.1103/PhysRevD.100.082004 |1 Agostini |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. D |v 100 |y 2019 |
| 999 | C | 5 | |1 Martyn |y 2021 |2 Crossref |o Martyn 2021 |
| 999 | C | 5 | |1 Kumaran |y 2021 |2 Crossref |o Kumaran 2021 |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|