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arxiv: 1311.4750 · v2 · pith:3ASA3YIVnew · submitted 2013-11-19 · ✦ hep-ex

Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

K. Abe , J. Adam , H. Aihara , T. Akiri , C. Andreopoulos , S. Aoki , A. Ariga , T. Ariga
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S. Assylbekov D. Autiero M. Barbi G. J. Barker G. Barr M. Bass M. Batkiewicz F. Bay S. W. Bentham V. Berardi B. E. Berger S. Berkman I. Bertram S. Bhadra F. d. M. Blaszczyk A. Blondel C. Bojechko S. Bordoni S. B. Boyd D. Brailsford A. Bravar C. Bronner N. Buchanan R. G. Calland J. Caravaca Rodr\'iguez S. L. Cartwright R. Castillo M. G. Catanesi A. Cervera D. Cherdack G. Christodoulou A. Clifton J. Coleman S. J. Coleman G. Collazuol K. Connolly L. Cremonesi A. Dabrowska I. Danko R. Das S. Davis P. de Perio G. De Rosa T. Dealtry S. R. Dennis C. Densham F. Di Lodovico S. Di Luise O. Drapier T. Duboyski K. Duffy F. Dufour J. Dumarchez S. Dytman M. Dziewiecki S. Emery A. Ereditato L. Escudero A. J. Finch L. Floetotto M. Friend Y. Fujii Y. Fukuda A. P. Furmanski V. Galymov A. Gaudin S. Giffin C. Giganti K. Gilje D. Goeldi T. Golan J. J. Gomez-Cadenas M. Gonin N. Grant D. Gudin D. R. Hadley A. Haesler M. D. Haigh P. Hamilton D. Hansen T. Hara M. Hartz T. Hasegawa N. C. Hastings Y. Hayato C. Hearty R. L. Helmer M. Hierholzer J. Hignight A. Hillairet A. Himmel T. Hiraki S. Hirota J. Holeczek S. Horikawa K. Huang A. K. Ichikawa K. Ieki M. Ieva M. Ikeda J. Imber J. Insler T. J. Irvine T. Ishida T. Ishii S. J. Ives K. Iyogi A. Izmaylov A. Jacob B. Jamieson R. A. Johnson J. H. Jo P. Jonsson C. K. Jung A. C. Kaboth T. Kajita H. Kakuno J. Kameda Y. Kanazawa D. Karlen I. Karpikov E. Kearns M. Khabibullin A. Khotjantsev D. Kielczewska T. Kikawa A. Kilinski J. Kim J. Kisiel P. Kitching T. Kobayashi L. Koch A. Kolaceke A. Konaka L. L. Kormos A. Korzenev K. Koseki Y. Koshio I. Kreslo W. Kropp H. Kubo Y. Kudenko S. Kumaratunga R. Kurjata T. Kutter J. Lagoda K. Laihem I. Lamont M. Laveder M. Lawe M. Lazos K. P. Lee C. Licciardi T. Lindner C. Lister R. P. Litchfield A. Longhin L. Ludovici M. Macaire L. Magaletti K. Mahn M. Malek S. Manly A. D. Marino J. Marteau J. F. Martin T. Maruyama J. Marzec E. L. Mathie V. Matveev K. Mavrokoridis E. Mazzucato M. McCarthy N. McCauley K. S. McFarland C. McGrew C. Metelko M. Mezzetto P. Mijakowski C. A. Miller A. Minamino O. Mineev S. Mine A. Missert M. Miura L. Monfregola S. Moriyama Th. A. Mueller A. Murakami M. Murdoch S. Murphy J. Myslik T. Nagasaki T. Nakadaira M. Nakahata T. Nakai K. Nakamura S. Nakayama T. Nakaya K. Nakayoshi D. Naples C. Nielsen M. Nirkko K. Nishikawa Y. Nishimura H. M. O'Keeffe R. Ohta K. Okumura T. Okusawa W. Oryszczak S. M. Oser R. A. Owen Y. Oyama V. Palladino V. Paolone D. Payne G. F. Pearce O. Perevozchikov J. D. Perkin Y. Petrov L. J. Pickard E. S. Pinzon Guerra C. Pistillo P. Plonski E. Poplawska B. Popov M. Posiadala J. -M. Poutissou R. Poutissou P. Przewlocki B. Quilain E. Radicioni P. N. Ratoff M. Ravonel M. A. M. Rayner A. Redij M. Reeves E. Reinherz-Aronis F. Retiere A. Robert P. A. Rodrigues P. Rojas E. Rondio S. Roth A. Rubbia D. Ruterbories R. Sacco K. Sakashita F. S\'anchez F. Sato E. Scantamburlo K. Scholberg J. Schwehr M. Scott Y. Seiya T. Sekiguchi H. Sekiya D. Sgalaberna M. Shiozawa S. Short Y. Shustrov P. Sinclair B. Smith R. J. Smith M. Smy J. T. Sobczyk H. Sobel M. Sorel L. Southwell P. Stamoulis J. Steinmann B. Still Y. Suda A. Suzuki K. Suzuki S. Y. Suzuki Y. Suzuki T. Szeglowski R. Tacik M. Tada S. Takahashi A. Takeda Y. Takeuchi H. K. Tanaka H. A. Tanaka M. M. Tanaka D. Terhorst R. Terri L. F. Thompson A. Thorley S. Tobayama W. Toki T. Tomura Y. Totsuka C. Touramanis T. Tsukamoto M. Tzanov Y. Uchida K. Ueno A. Vacheret M. Vagins G. Vasseur T. Wachala A. V. Waldron C. W. Walter D. Wark M. O. Wascko A. Weber R. Wendell R. J. Wilkes M. J. Wilking C. Wilkinson Z. Williamson J. R. Wilson R. J. Wilson T. Wongjirad Y. Yamada K. Yamamoto C. Yanagisawa S. Yen N. Yershov M. Yokoyama T. Yuan A. Zalewska J. Zalipska L. Zambelli K. Zaremba M. Ziembicki E. D. Zimmerman M. Zito J. \.Zmuda (for the T2K collaboration)
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The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3$\sigma$ when compared to 4.92 $\pm$ 0.55 expected background events. In the PMNS mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles $\theta_{12}$, $\theta_{23}$, $\theta_{13}$, a mass difference $\Delta m^2_{32}$ and a CP violating phase $\delta_{\mathrm{CP}}$. In this neutrino oscillation scenario, assuming $|\Delta m^2_{32}| = 2.4 \times 10^{-3}$ $\rm eV^2$, $\sin^2 \theta_{23} = 0.5$, and $\Delta m^2_{32} >0$ ($\Delta m^2_{32} <0$), a best-fit value of $\sin^2 2 \theta_{13}$ = $0.140^{+0.038}_{-0.032}$ ($0.170^{+0.045}_{-0.037}$) is obtained at $\delta_{\mathrm{CP}}=0$. When combining the result with the current best knowledge of oscillation parameters including the world average value of $\theta_{13}$ from reactor experiments, some values of $\delta_{\mathrm{CP}}$ are disfavored at the 90% CL.

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