Home > Publications database > Limiting the effective magnetic moment of solar neutrinos with the Borexino detector > print |
001 | 890234 | ||
005 | 20250512115731.0 | ||
024 | 7 | _ | |a 10.1088/1742-6596/1342/1/012033 |2 doi |
024 | 7 | _ | |a 1742-6588 |2 ISSN |
024 | 7 | _ | |a 1742-6596 |2 ISSN |
024 | 7 | _ | |a 2128/27068 |2 Handle |
024 | 7 | _ | |a WOS:001432953400033 |2 WOS |
037 | _ | _ | |a FZJ-2021-00821 |
082 | _ | _ | |a 530 |
100 | 1 | _ | |a Ludhova, Livia |0 P:(DE-Juel1)168122 |b 0 |e Corresponding author |u fzj |
111 | 2 | _ | |a TAUP 2017 |c Sudbury |d 2017-07-24 - 2017-07-28 |w Canada |
245 | _ | _ | |a Limiting the effective magnetic moment of solar neutrinos with the Borexino detector |
260 | _ | _ | |a Bristol |c 2020 |b IOP Publ.87703 |
264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
264 | _ | 1 | |3 print |2 Crossref |b IOP Publishing |c 2020-01-01 |
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 1611672525_2352 |2 PUB:(DE-HGF) |
520 | _ | _ | |a Borexino has provided an updated upper limit on the effective neutrino magnetic moment of solar neutrinos μβα < 2.8 x 10−11 μऔ at 90% C.L. This result represents nearly a factor of two improvement with respect to the previous result based on 192 days of the Phase-I data. The current analysis has been performed using 1291.5 days exposure of the Phase-II data, characterized by a further improved level of radio-purity of liquid scintillator. Another key ingredient of the new analysis, lowering the threshold from 260 to 186 keV, was possible thanks to a better understanding of the detector-response function at low energies. The global spectral fit was preformed up to 2970 keV energy, using constraints on the sum of the solar neutrino fluxes implied by the radiochemical gallium experiments. From the limit for the effective neutrino magnetic moment, new limits for the magnetic moments of the neutrino flavour states were derived. |
536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF3-612) |0 G:(DE-HGF)POF3-612 |c POF3-612 |f POF III |x 0 |
542 | _ | _ | |i 2020-01-01 |2 Crossref |u http://creativecommons.org/licenses/by/3.0/ |
542 | _ | _ | |i 2020-01-01 |2 Crossref |u https://iopscience.iop.org/info/page/text-and-data-mining |
588 | _ | _ | |a Dataset connected to CrossRef |
700 | 1 | _ | |a Borexino collaboration |0 P:(DE-HGF)0 |b 1 |
773 | 1 | 8 | |a 10.1088/1742-6596/1342/1/012033 |b IOP Publishing |d 2020-01-01 |n 1 |p 012033 |3 journal-article |2 Crossref |t Journal of Physics: Conference Series |v 1342 |y 2020 |x 1742-6588 |
773 | _ | _ | |a 10.1088/1742-6596/1342/1/012033 |g Vol. 1342, p. 012033 - |0 PERI:(DE-600)2166409-2 |n 1 |p 012033 |t Journal of physics / Conference Series |v 1342 |y 2020 |x 1742-6588 |
856 | 4 | _ | |u https://juser.fz-juelich.de/record/890234/files/Ludhova_2020_J._Phys.%20_Conf._Ser._1342_012033.pdf |y OpenAccess |
909 | C | O | |o oai:juser.fz-juelich.de:890234 |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)168122 |
913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Universum |1 G:(DE-HGF)POF3-610 |0 G:(DE-HGF)POF3-612 |3 G:(DE-HGF)POF3 |2 G:(DE-HGF)POF3-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
914 | 1 | _ | |y 2020 |
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 | 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 Bellini |y 2011 |2 Crossref |o Bellini 2011 |
999 | C | 5 | |a 10.1103/PhysRevLett.108.051302 |1 Bellini |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. Lett. |v 108 |y 2012 |
999 | C | 5 | |a 10.1038/nature13702 |9 -- missing cx lookup -- |1 Bellini |p 383 - |2 Crossref |t Nature |v 512 |y 2014 |
999 | C | 5 | |a 10.1103/PhysRevD.82.033006 |1 Bellini |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. D |v 82 |y 2010 |
999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
999 | C | 5 | |a 10.1007/JHEP08(2013)038 |9 -- missing cx lookup -- |1 Bellini |p 038 - |2 Crossref |t JHEP |v 1308 |y 2013 |
999 | C | 5 | |a 10.1134/S1547477113020027 |9 -- missing cx lookup -- |1 Beda |p 139 - |2 Crossref |t Phys.Part. and Nucl.Lett. |v 10 |y 2013 |
999 | C | 5 | |1 Wong |y 2007 |2 Crossref |o Wong 2007 |
999 | C | 5 | |1 Liu |y 2004 |2 Crossref |o Liu 2004 |
999 | C | 5 | |1 Bellini |y 2008 |2 Crossref |o Bellini 2008 |
999 | C | 5 | |1 Agostini |y 2017 |2 Crossref |o Agostini 2017 |
999 | C | 5 | |1 Raffelt |y 1988 |2 Crossref |o Raffelt 1988 |
999 | C | 5 | |a 10.1016/j.astropartphys.2015.03.006 |9 -- missing cx lookup -- |1 Arceo-Díaz |p 1 - |2 Crossref |t Astropart. Phys. |v 70 |y 2015 |
999 | C | 5 | |a 10.1103/PhysRevD.89.112007 |1 Bellini |9 -- missing cx lookup -- |2 Crossref |t Phys. Rev. D |v 89 |y 2014 |
999 | C | 5 | |a 10.1103/PhysRevC.80.015807 |9 -- missing cx lookup -- |1 Abdurashitov |p 1 - |2 Crossref |t Phys. Rev. C |v 80 |y 2009 |
999 | C | 5 | |1 Patrignani |y 2016 |2 Crossref |o Patrignani 2016 |
Library | Collection | CLSMajor | CLSMinor | Language | Author |
---|