Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV

Bronner, C.; Haga, Y.; Hayato, Y.; Ikeda, M.; Iyogi, K.; Kameda, J.; Kato, Y.; Kishimoto, Y.; Marti, Ll.; Miura, Makoto; Moriyama, S.; Nakahata, M.; Nakajima, Tetsuo; Nakano, Y.; Nakayama, S.; Okajima, Y.; Orii, A.; Pronost, G.; Sekiya, H.; Shiozawa, M.; Sonoda, Y.; Takeda, Atsushi; Takenaka, A.; Tasaka, S.; Tomura, T.; Akutsu, R.; Irvine, T. J.; Kajita, T.; Kametani, I.; Kaneyuki, K.; Nishimura, Y.; Okumura, K.; Richard, E.; Tsui, K. M.; Labarga, L.; Fernández, P.; Blaszczyk, F. d. M.; Gustafson, J.; Kachulis, C.; Kearns, E.; Raaf, J. L.; Stone, James L.; Sulak, L.; Berkman, S.; Tobayama, S.; Goldhaber, M.; Carminati, G.; Elnimr, M.; Kropp, W. R.; Mine, S.; Locke, S.; Renshaw, A.; Smy, M. B.; Sobel, H. W.; Takhistov, Volodymyr; Weatherly, P.; Ganezer, K. S.; Hartfiel, B. L.; Hill, J.; Hồng, Nguyễn Thị; Kim, J. Y.; Lim, I. T.; Park, R. G.; Akiri, T.; Himmel, A.; Li, Z.; O’Sullivan, Erin; Scholberg, K.; Walter, C. W.; Wongjirad, T.; Ishizuka, T.; Nakamura, T.; Jang, J. S.; Choi, K.; Learned, J. G.; Matsuno, S.; Smith, S. N.; Amey, Jake Lewis; Litchfield, R. P.; Y., W.; Uchida, Y.; Wascko, M. O.; Cao, S.; Friend, M.; Hasegawa, T.; Ishida, Toru; Ishii, T.; Kobayashi, T.; Nakadaira, T.; Nakamura, K.; Oyama, Y.; Sakashita, K.; Sekiguchi, T.; Tsukamoto, T.; Abe, K.; Hasegawa, M.; Suzuki, A.; Takeuchi, Y.; Yano, T.; Hayashino, T.; Hirota, S.; Huang, K.; Ieki, K.; Jiang, M.; Kikawa, T.; Nakamura, K.; Nakaya, T.; Patel, N. D.; Suzuki, K.; Takahashi, Sentaro; Wendell, R.; Anthony, L. H. V.; McCauley, N.; Pritchard, A.; Fukuda, Y.; Itow, Y.; Mitsuka, G.; Murase, M.; Muto, Fumihito; Suzuki, T.; Mijakowski, P.; Frankiewicz, K.; Hignight, J.; Imber, J.; Jung, C. K.; Li, X.; Palomino, J. L.; Santucci, G.; Vilela, C.; Wilking, M. J.; Yanagisawa, C.; Ito, S.; Fukuda, Daisuke; Ishino, H.; Kayano, T.; Kibayashi, A.; Koshio, Y.; Mori, Takaaki; Nagata, Hiroshi; Sakuda, M.; Xu, Chenyuan; Kuno, Y.; Wark, D.; Lodovico, F. Di; Richards, B.; Tacik, R.; Kim, S. B.; Cole, A. A.; Thompson, L. F.; Okazawa, H.; Choi, Y.; Ito, K.; Nishijima, K.; Koshiba, M.; Totsuka, Y.; Suda, Y.; Yokoyama, M.; Calland, R. G.; Hartz, M.; Martens, K.; Quilain, B.; Simpson, C.; Suzuki, Yoshihiro; Vagins, M.; Hamabe, D.; Kuze, M.; Yoshida, Tadashi; Ishitsuka, M.; Martin, J. F.; Nantais, C.; Perio, P. de; Tanaka, Hirohisa; Konaka, A.; Chen, S.; Wan, L.; Zhang, Y.; Wilkes, R. J.; Minamino, A.

doi:10.1103/physrevd.97.072001

Cited by 221 publications

(233 citation statements)

References 71 publications

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“…Figure 10 shows the 1, 2, and 3σ two-dimensional contours for Δm 2 32 and sin 2 θ 23 , separately for each mass hierarchy. Figure 11 shows a comparison of 90% confidence level contours for these parameters in the normal mass hierarchy for NOvA, T2K [7], MINOS [6], IceCube [57], and Super-Kamiokande [58] range 0.96 to 1.00 in sin 2 2θ 23 , which is the variable directly measured in ν μ → ν μ oscillations. Figure 12 shows the analogous contours to those of Fig.…”

Section: Best Fitsmentioning

confidence: 99%

New constraints on oscillation parameters fromνeappearance andνμdisappearance in the NOvA experiment

Acero¹,

Adamson²,

Aliaga³

et al. 2018

Phys. Rev. D

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180

192

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We present updated results from the NOvA experiment for ν μ → ν μ and ν μ → ν e oscillations from an exposure of 8.85 × 10 20 protons on target, which represents an increase of 46% compared to our previous publication. The results utilize significant improvements in both the simulations and analysis of the data. A joint fit to the data for ν μ disappearance and ν e appearance gives the best-fit point as normal mass hierarchy, Δm 2 32 ¼ 2.44 × 10 −3 eV 2 =c 4 , sin 2 θ 23 ¼ 0.56, and δ CP ¼ 1.21π. The 68.3% confidence intervals in the normal mass hierarchy are Δm 2 32 ∈ ½2.37; 2.52 × 10 −3 eV 2 =c 4 , sin 2 θ 23 ∈ ½0.43; 0.51 ∪ ½0.52; 0.60, and δ CP ∈ ½0; 0.12π ∪ ½0.91π; 2π. The inverted mass hierarchy is disfavored at the 95% confidence level for all choices of the other oscillation parameters.

show abstract

Section: Best Fitsmentioning

confidence: 99%

New constraints on oscillation parameters fromνeappearance andνμdisappearance in the NOvA experiment

Acero¹,

Adamson²,

Aliaga³

et al. 2018

Phys. Rev. D

Self Cite

180

192

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“…The current fit from various experiments (e.g. Super-Kamiokande [27], T2K [28], NOvA [29]) gives above 3-σ preference for normal over inverted ordering. A 3-σ rejection of the wrong mass ordering will be obtained in Hyper-K [26] after five years of data taking.…”

Section: Predictionsmentioning

confidence: 80%

Tribimaximal mixing in the SU(5)×T13 texture

et al. 2020

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We extend the recently proposed SU (5) × T 13 model for the asymmetric texture to the up-type quark and Seesaw sectors. The hierarchical up-type quark masses are generated from higher-dimensional operators involving family-singlet Higgses, gauge-singlet familons, and vector-like messengers. The complex-Tribimaximal (TBM) Seesaw mixing arises from the vacuum structure of a minimal number of familons, resulting in an alignment between the Yukawa and Majorana matrices of the Seesaw formula. Introducing four right-handed neutrinos, normal ordering of the light neutrino masses is obtained, with m ν1 = 27.6 meV, m ν2 = 28.9 meV and m ν3 = 57.8 meV. Their sum almost saturates Planck's cosmological upper bound (120 meV). The right-handed neutrino masses are expressed in terms of two parameters for a particular choice of familon vacuum alignment. We predict the¨CP Jarlskog-Greenberg invariant to be |J | = 0.028, consistent with the current PDG estimate, and Majorana invariants |I 1 | = 0.106 and |I 2 | = 0.011. A sign ambiguity in the model parameters leads to two possibilities for the invariant mass parameter |m ββ |: 13.02 meV or 25.21 meV, both within an order of magnitude of the most rigorous experimental upper limit (61-165 meV). *

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“…5 in Ref. [34], respectively). In the case of e-like events, we add both the ν e andν e samples as well.…”

mentioning

confidence: 86%

“…5 of ref. [34]. We use both the µand e-like fully-contained multi-GeV events, adding the single-and multi-ring samples together (labeled as "multi-GeV" and "multi-ring" in Fig.…”

mentioning

confidence: 99%

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New constraints on heavy neutral leptons from Super-Kamiokande data

Coloma¹,

Hernández²,

Muñoz³

et al. 2020

Eur. Phys. J. C

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Heavy neutral leptons are predicted in many extensions of the Standard Model with massive neutrinos. If kinematically accessible, they can be copiously produced from kaon and pion decays in atmospheric showers, and subsequently decay inside large neutrino detectors. We perform a search for these long-lived particles using Super-Kamiokande multi-GeV neutrino data and derive stringent limits on the mixing with electron, muon and tau neutrinos as a function of the long-lived particle mass. We also present the limits on the branching ratio versus lifetime plane, which are helpful in determining the constraints in non-minimal models where the heavy neutral leptons have new interactions with the Standard Model.

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Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV

Cited by 221 publications

References 71 publications

New constraints on oscillation parameters fromνeappearance andνμdisappearance in the NOvA experiment

New constraints on oscillation parameters fromνeappearance andνμdisappearance in the NOvA experiment

Tribimaximal mixing in the SU(5)×T13 texture

New constraints on heavy neutral leptons from Super-Kamiokande data

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