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Related papers: Bounds on $\nu_{\mu}$ Oscillations from Atmospheri…

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A lower bound on $\Delta m^{2}$ for atmospheric neutrino oscillations can be obtained from the global value of $R$ at a given energy. This bound may be more reliable than one based on the observed isotropy. Some global values of $R$ imply…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. M. LoSecco

Within the standard $3\nu$ framework, we discuss updated bounds on the leading oscillation parameters related to the $(\nu_1,\,\nu_2)$ states, namely, the squared mass difference $\delta m^2=m^2_2-m^2_1$ and the mixing parameter…

High Energy Physics - Phenomenology · Physics 2025-11-27 Francesco Capozzi , Eligio Lisi , Francesco Marcone , Antonio Marrone , Antonio Palazzo

This paper presents the recent results from Super-Kamiokande atmospheric neutrinos and from K2K accelerator neutrinos. Both results show the signal of neutrino oscillation, and provide new and precise information of oscillation parameters.…

High Energy Physics - Experiment · Physics 2007-05-23 T. Nakaya

Limits on $\nu_\mu \to \nu_e$ and $\bar\nu_\mu \to \bar\nu_e$ oscillations are extracted using the NuTeV detector with sign-selected $\nu_\mu$ and $\nub_\mu$ beams. In $\nub_\mu$ mode, for the case of $\sin^2 2\alpha = 1$, $\Delta m^2 >…

By combining experimental constraints from atmospheric and solar neutrino oscillations and the tritium beta decay endpoint, we infer upper limits of 4.4 eV on the $\nu_\mu$ and $\nu_\tau$ masses, if the universe consists of three neutrinos.…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , T. J. Weiler , K. Whisnant

In a previous paper [1], we presented a three-flavour oscillation analysis of the solar neutrino measurements and of the first data from the KamLAND experiment, in terms of the relevant mass-mixing parameters (delta m^2, theta_12,…

High Energy Physics - Phenomenology · Physics 2009-10-07 G. L. Fogli , E. Lisi , A. Marrone , D. Montanino , A. Palazzo , A. M. Rotunno

The energy spectrum of neutrino-induced upward-going muons in MACRO was analysed in terms of relativity principles violating effects, keeping standard mass-induced atmospheric neutrino oscillations as the dominant effect. The data disfavor…

We perform a detailed analysis of the capabilities of the MINOS, ICARUS and OPERA experiments to measure neutrino oscillation parameters at the atmospheric scale with their data taken separately and in combination. MINOS will determine…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , A. M. Gago , D. Marfatia , W. J. C. Teves , B. P. Wood , R. Zukanovich Funchal

We derive predictions for the Nadir angle (theta_n) dependence of the ratio Nmu-/Nmu+ of the rates of the mu- and mu+ multi-GeV events, and for the mu- - mu+ event rate asymmetry, A_{mu-mu+}=[Nmu- - Nmu+]/[Nmu- + Nmu+], in iron-magnetized…

High Energy Physics - Phenomenology · Physics 2010-04-05 Sergio Palomares-Ruiz , S. T. Petcov

We derive new bounds on the Dirac mass of the tau and muonic neutrinos. By solving the kinetic equation for the rate of energy deposition due to helicity flipping processes and imposing the constraint that the number of effective species…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. D. Dolgov , K. Kainulainen , I. Z. Rothstein

We discuss the possibility for matter effects in the three-neutrino oscillations of the atmospheric nu_e (bar{nu}_e) and nu_mu (bar{nu}_mu), driven by one neutrino mass squared difference, |Delta m2_{31}| >> Delta m2_{21}, to be observable…

High Energy Physics - Phenomenology · Physics 2007-05-23 Jose Bernabeu , Sergio Palomares-Ruiz

We have performed a likelihood analysis of the recent data on the Cosmic Microwave Background Radiation (CMBR) anisotropy taken by the Boomerang experiment. We find that this data places a strong upper bound on the radiation density present…

Astrophysics · Physics 2009-10-31 Steen Hannestad

The energy spectrum of neutrino-induced upward-going muons in MACRO has been analysed in terms of relativity principles violating effects, keeping standard mass-induced atmospheric neutrino oscillations as the dominant source of $\nu_{\mu}…

High Energy Physics - Experiment · Physics 2008-11-26 M. Cozzi

Limits on $\nu_\mu (\overline{\nu}_\mu) \to \nu_e (\overline{\nu}_e)$ oscillations based on a statistical separation of $\nu_e N$ charged current interactions in the CCFR detector at Fermilab are presented. $\nu_e$ interactions are…

High Energy Physics - Experiment · Physics 2012-08-27 NuTeV Collaboration , A. Romosan

We derive predictions for the Nadir angle (theta(n)) dependence of the ratio N(mu)/N(e) of the rates of the mu-like and e-like multi-GeV events measured in water-Cerenkov detectors in the case of 3-neutrino oscillations of the atmospheric…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. Bernabeu , Sergio Palomares-Ruiz , S. T. Petcov

We present the constraints on neutrino oscillation parameters $\Delta m^2_{\odot}$ and $\theta_{\odot}$ governing the solar neutrino oscillations from two generation analysis of solar and KamLAND data. We include the latest 766.3 ton year…

High Energy Physics - Phenomenology · Physics 2014-11-18 Srubabati Goswami , Abhijit Bandyopadhyay , Sandhya Choubey

The observation of the recent electron neutrino appearance in a muon neutrino beam and the high-precision measurement of the mixing angle $\theta_{13}$ have led to a re-evaluation of the physics potential of the T2K long-baseline neutrino…

High Energy Physics - Experiment · Physics 2015-04-01 K. Abe , J. Adam , H. Aihara , T. Akiri , C. Andreopoulos , S. Aoki , A. Ariga , S. Assylbekov , D. Autiero , M. Barbi , G. J. Barker , G. Barr , P. Bartet-Friburg , M. Bass , M. Batkiewicz , F. Bay , V. Berardi , B. E. Berger , S. Berkman , 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 , D. Dewhurst , F. Di Lodovico , S. Di Luise , O. Drapier , T. Duboyski , K. Duffy , J. Dumarchez , S. Dytman , M. Dziewiecki , S. Emery-Schrenk , A. Ereditato , L. Escudero , T. Feusels , A. J. Finch , G. A. Fiorentini , M. Friend , Y. Fujii , Y. Fukuda , A. P. Furmanski , V. Galymov , A. Garcia , S. Giffin , C. Giganti , K. Gilje , D. Goeldi , T. Golan , M. Gonin , N. Grant , D. Gudin , D. R. Hadley , L. Haegel , A. Haesler , M. D. Haigh , P. Hamilton , D. Hansen , T. Hara , M. Hartz , T. Hasegawa , N. C. Hastings , T. Hayashino , 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 , E. Iwai , K. Iwamoto , K. Iyogi , A. Izmaylov , A. Jacob , B. Jamieson , R. A. Johnson , S. Johnson , J. H. Jo , P. Jonsson , C. K. Jung , M. Kabirnezhad , A. C. Kaboth , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , T. Katori , E. Kearns , M. Khabibullin , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Kim , S. King , J. Kisiel , P. Kitching , T. Kobayashi , L. Koch , T. Koga , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , Y. Koshio , W. Kropp , H. Kubo , Y. Kudenko , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , I. Lamont , E. Larkin , M. Laveder , M. Lawe , M. Lazos , T. Lindner , C. Lister , R. P. Litchfield , A. Longhin , J. P. Lopez , L. Ludovici , L. Magaletti , K. Mahn , M. Malek , S. Manly , A. D. Marino , J. Marteau , J. F. Martin , P. Martins , S. Martynenko , T. Maruyama , V. Matveev , K. Mavrokoridis , E. Mazzucato , M. McCarthy , N. McCauley , K. S. McFarland , C. McGrew , A. Mefodiev , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , A. Missert , M. Miura , S. Moriyama , Th. A. Mueller , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nakadaira , M. Nakahata , K. G. Nakamura , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , C. Nantais , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , J. Nowak , H. M. O'Keeffe , R. Ohta , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , T. Ovsyannikova , R. A. Owen , Y. Oyama , V. Palladino , J. L. Palomino , V. Paolone , D. Payne , O. Perevozchikov , J. D. Perkin , Y. Petrov , L. Pickard , E. S. Pinzon Guerra , C. Pistillo , P. Plonski , E. Poplawska , B. Popov , M. Posiadala-Zezula , 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 , C. Riccio , 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 , S. Schoppmann , J. Schwehr , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , R. Shah , F. Shaker , M. Shiozawa , S. Short , Y. Shustrov , P. Sinclair , B. 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 , 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 , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , A. V. Waldron , K. Wakamatsu , C. W. Walter , D. Wark , W. Warzycha , 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 , T. Yano , S. Yen , N. Yershov , M. Yokoyama , K. Yoshida , T. Yuan , M. Yu , A. Zalewska , J. Zalipska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

The apparent attenuation of muon neutrinos relative to electron neutrinos is a bit too low to be compatible with the most popular values of $\Delta m^{2}$. Fits to $R(E_{\nu})$ favor values of $\Delta m^{2}>0.1$ eV$^{2}$. The fit minimized…

High Energy Physics - Phenomenology · Physics 2009-10-31 J. M. LoSecco

We give predictions for the up-down asymmetry in the Nadir angle dependence of the ratio Nmu/Ne of the rates of the mu-like and e-like multi-GeV events measured in water-Cerenkov detectors (Super-Kamiokande, etc.) in the case of 3-neutrino…

High Energy Physics - Phenomenology · Physics 2016-12-07 S. T. Petcov , Sergio Palomares-Ruiz
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