A search for flavor-changing non-standard neutrino interactions by MINOS

P Adamson, G Barr,M Bishai,A Blake,G J Bock,D Bogert,S V Cao,D Cherdack,S Childress,J A B Coelho,L A Corwin,D Croninhennessy,J K De Jong, A V Devan, N E Devenish,M V Diwan,C Escobar,J J Evans, E Falk,G J Feldman, M V Frohne, H R Gallagher,R A Gomes, M C Goodman,P Gouffon, N Graf, R Gran,K Grzelak,A Habig,J Hartnell,R Hatcher,A Himmel, A Holin, J Hylen, G M Irwin, Z Isvan,C James, D A Jensen, T Kafka,S Kasahara, G Koizumi, M Kordosky,A Kreymer, K Lang,J Ling, P J Litchfield,P Lucas,W A Mann,M L Marshak,M Mathis,N Mayer, M M Medeiros,R Mehdiyev, J R Meier,M D Messier,W H Miller,S R Mishra,S Moed Sher,C D Moore,L Mualem, S Mufson,J Musser, D Naples,J K Nelson, H B Newman,R J Nichol, J A Nowak, W P Oliver, M Orchanian,R B Pahlka, J Paley, R B Patterson, G Pawloski, S Phanbudd,R Plunkett, Xingzhi Qiu,A Radovic,B Rebel,C Rosenfeld, H A Rubin,M C Sanchez,J Schneps,A Schreckenberger, P Schreiner,R K Sharma,Ana Luiza Lima Sousa,N Tagg,R L Talaga,J P Thomas,Mark Thomson,R Toner,D Torretta, G Tzanakos, J Urheim,P Vahle,B Viren, Andreas P M Weber,R Webb,Christopher G White

PHYSICAL REVIEW D(2013)

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摘要
We report new constraints on flavor-changing non-standard neutrino interactions from the MINOS experiment, in which neutrino versus antineutrino interactions can be distinguished on an event-by-event basis. We analyzed a combined set of beam neutrino and antineutrino data from the well-understood NuMI beam, and found no evidence for deviations from standard neutrino mixing. The observed energy spectra constrain the non-standard neutrino interactions parameter to the range -0.20 < epsilon(mu tau) < 0.07 (90%C.L.).
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关键词
MINOS,Neutrino oscillation,Neutrino,Solar neutrino problem,Measurements of neutrino speed,Solar neutrino,Fermilab,NuMI,Particle physics,Nuclear physics,Physics
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