2017
DOI: 10.1103/physrevd.96.092006
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Measurement of neutrino and antineutrino oscillations by the T2K experiment including a new additional sample ofνeinteractions at the far detector

Abstract: The T2K experiment reports an updated analysis of neutrino and antineutrino oscillations in appearance and disappearance channels. A sample of electron neutrino candidates at Super-Kamiokande in which a pion decay has been tagged is added to the four single-ring samples used in previous T2K oscillation analyses. Through combined analyses of these five samples, simultaneous measurements of four oscillation parameters, jΔm 2 32 j, sin 2 θ 23 , sin 2 θ 13 , and δ CP and of the mass ordering are made. A set of stu… Show more

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Cited by 150 publications
(156 citation statements)
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“…Figure 2 (right) depicts the NOvA 90% C.L. contour in comparison to previous results from MINOS [9] and T2K [10]. For a full discussion of the details of the muon neutrino disappearance analysis refer to the publication in Ref.…”
Section: Muon Neutrino Disappearancementioning
confidence: 99%
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“…Figure 2 (right) depicts the NOvA 90% C.L. contour in comparison to previous results from MINOS [9] and T2K [10]. For a full discussion of the details of the muon neutrino disappearance analysis refer to the publication in Ref.…”
Section: Muon Neutrino Disappearancementioning
confidence: 99%
“…Right: NOvA's best-fit (black dots) points and allowed 90% C.L. regions compared to previous results from MINOS [9] and T2K [10] (dashed curves).…”
Section: Muon Neutrino Disappearancementioning
confidence: 99%
“…The results recently published by T2K are ∆m 2 32 = (2.54 ± 0.08) × 10 −3 eV 2 and sin 2 θ 23 = 0.55 +0.05 −0.09 [47], both for a normal mass-hierarchy. Results for the inverted hierarchy are similar (up to ∆m 2 32 approximately changing sign).…”
Section: Neutrino Parameter Measurementsmentioning
confidence: 99%
“…Neutrino oscillation parameters are mostly constrained by solar neutrino experiments [40][41][42][43][44][45], the SuperKamiokande atmospheric neutrino data [37], and accelerator data from MINOS [46], T2K [47], and the NuMI Off-Axis ν e Appearance Experiment (NOνA) [48]. These imply the existence of two hierarchical mass-squared differences ∆m 2 21 and ∆m 2 32 and three nonzero mixing angles θ 13 , θ 12 , θ 23 .…”
Section: Neutrino Parameter Measurementsmentioning
confidence: 99%
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