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dc.contributor.authorAlbert, Arthur
dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAndré, Michel
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnton, Gisela
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorAubert, J.-J.
dc.contributor.authorAublin, J.
dc.contributor.authorBaret, Bruny
dc.contributor.authorBasa, Stéphane
dc.contributor.authorBelhorma, Bouchra
dc.contributor.authorBendahman, Meriem
dc.contributor.authorBertin, Vincent
dc.contributor.authorBiagi, S.
dc.contributor.otherCentre Tecnològic de Vilanova i la Geltrú
dc.date.accessioned2022-09-13T17:32:12Z
dc.date.available2022-09-13T17:32:12Z
dc.date.issued2022-07-08
dc.identifier.citationAlbert, A. [et al.]. Search for non-standard neutrino interactions with 10 years of ANTARES data. "Journal of high energy physics", 8 Juliol 2022, vol. 2022, núm. 48, p. 1-22.
dc.identifier.issn1029-8479
dc.identifier.otherhttps://arxiv.org/abs/2112.14517
dc.identifier.urihttp://hdl.handle.net/2117/372728
dc.description.abstractNon-standard interactions of neutrinos arising in many theories beyond the Standard Model can significantly alter matter effects in atmospheric neutrino propagation through the Earth. In this paper, a search for deviations from the prediction of the standard 3-flavour atmospheric neutrino oscillations using the data taken by the ANTARES neutrino telescope is presented. Ten years of atmospheric neutrino data collected from 2007 to 2016, with reconstructed energies in the range from ~16 GeV to 100 GeV, have been analysed. A log-likelihood ratio test of the dimensionless coefficients eµt and ett-eµµ does not provide clear evidence of deviations from standard interactions. For normal neutrino mass ordering, the combined fit of both coefficients yields a value 1.7s away from the null result. However, the 68% and 95% confidence level intervals for eµt and ett-eµµ, respectively, contain the null value. Best fit values, one standard deviation errors and bounds at the 90% confidence level for these coefficients are given for both normal and inverted mass orderings. The constraint on eµt is among the most stringent to date and it further restrains the strength of possible non-standard interactions in the µ-t sector.
dc.format.extent22 p.
dc.language.isoeng
dc.publisherSpringer
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshNeutrino astrophysics
dc.subject.otherNeutrino Detectors and Telescopes (experiments)
dc.titleSearch for non-standard neutrino interactions with 10 years of ANTARES data
dc.typeArticle
dc.subject.lemacNeutrins
dc.subject.lemacAstrofísica
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1007/JHEP07(2022)048
dc.relation.publisherversionhttps://link.springer.com/article/10.1007/JHEP07(2022)048
dc.rights.accessOpen Access
local.identifier.drac34208344
dc.description.versionPostprint (published version)
local.citation.authorAlbert, A.; Alves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bendahman, M.; Bertin, V.; Biagi, S.
local.citation.publicationNameJournal of high energy physics
local.citation.volume2022
local.citation.number48
local.citation.startingPage1
local.citation.endingPage22


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