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The exchange of a pair of low-mass neutrinos between electrons, protons and neutrons produces a "long-range" $1/r^5$ potential, which can be sought for in phenomena originating on the atomic and sub-atomic length scales. We calculate the…

Atomic Physics · Physics 2018-06-06 Yevgeny V. Stadnik

We suggest a would-be solution to the solar neutrino tension why solar neutrinos appear to mix differently from reactor antineutrinos, in theoretical respect. To do that, based on an extended theory with light sterile neutrinos added we…

High Energy Physics - Phenomenology · Physics 2021-03-31 Y. H. Ahn

In the context of the seesaw mechanism, it is natural that the large solar and atmospheric neutrino mixing angles originate separately from large 2 by 2 mixings in the neutrino and charged-lepton sectors, respectively, and large mixing in…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , Martti Raidal , T. Yanagida

Within the framework of three-flavor neutrino oscillations, we consider the physics potential of \nu_e --> \nu_\mu appearance and \nu_\mu --> \nu_\mu survival measurements at a neutrino factory for a leading oscillation scale \delta m^2 ~…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , S. Geer , R. Raja , K. Whisnant

We present the results of a Bayesian analysis of solar neutrino data in terms of nu_e->nu_{mu,tau} oscillations, independent from the Standard Solar Model predictions for the solar neutrino fluxes. We show that such a model independent…

High Energy Physics - Phenomenology · Physics 2009-11-07 M. V. Garzelli , C. Giunti

The triplet scalars $(\Delta=\Delta^{++},\Delta^{+},\Delta^{0})$, utilized in the so-called Type-II seesaw model to explain the lightness of neutrinos, would generate nonstandard interactions (NSI) for neutrino propagating in matter. We…

High Energy Physics - Phenomenology · Physics 2018-06-06 Katri Huitu , Timo J. Kärkkäinen , Jukka Maalampi , Sampsa Vihonen

We study lepton flavor violating (LFV) tau and B decays in models with heavy neutrinos to constrain the mixing matrix parameters U_{tau N}. We find that the best current constraints when the heavy neutrinos are purely left-handed come from…

High Energy Physics - Phenomenology · Physics 2009-11-10 Xiao-Gang He , G. Valencia , Yili Wang

We study three-flavor collective neutrino transformations in the dense-neutrino region above the neutrino sphere of a supernova core. We find that two-flavor conversions driven by the atmospheric mass difference and the 13-mixing angle…

Astrophysics · Physics 2008-12-18 Andreu Esteban-Pretel , Sergio Pastor , Ricard Tomas , Georg G. Raffelt , Gunter Sigl

The observed flavor oscillations of solar and atmospheric neutrinos determine several elements of the leptonic mixing matrix, but leave open the small mixing angle Theta_13, a possible CP-violating phase, the mass ordering, the absolute…

Astrophysics · Physics 2017-08-23 G. G. Raffelt

In this short review we discuss the notion of lepton numbers. The strong evidence in favor of neutrino oscillations obtained recently in the Super-Kamiokande atmospheric neutrino experiment and in solar neutrino experiments imply that the…

High Energy Physics - Phenomenology · Physics 2009-11-07 S. M. Bilenky , C. Giunti

We study experimental and cosmological constraints on the extension of the Standard Model by three right handed neutrinos with masses between those of the pion and W boson. We combine for the first time direct, indirect and cosmological…

High Energy Physics - Phenomenology · Physics 2017-08-07 Marco Drewes , Björn Garbrecht

A new atmospheric neutrino oscillation tool which utilizes full three neutrino oscillation probabilities and a full three neutrino treatment of the MSW effect is combined with a standard analysis of the K2K, MINOS, and CHOOZ data to examine…

Nuclear Theory · Physics 2009-08-20 J. E. Roa , D. C. Latimer , D. J. Ernst

Deviations from expectations have been claimed for solar, atmospheric and high energy prompt neutrinos from charm decay. This information, supplemented only by the existing very good upper limits for oscillations of the $\nu_{\mu}$ at…

High Energy Physics - Phenomenology · Physics 2011-05-23 G. Conforto , A. Marchionni , F. Martelli , F. Vetrano , M. Lanfranchi , G. Torricelli-Ciamponi

The next-generation neutrino oscillation experiments would be sensitive to the new neutrino interactions that would strengthen the search for physics beyond the Standard Model. In this context, we explore the capabilities of the two leading…

High Energy Physics - Phenomenology · Physics 2025-01-28 Sanjib Kumar Agarwalla , Mauricio Bustamante , Masoom Singh , Pragyanprasu Swain

We perform a comprehensive analysis of neutrinoless double beta decay and its interplay with low-energy flavor observables in a radiative neutrino mass model with scalar leptoquarks $S_1(\bar{3},1,1/3)$ and $\widetilde{R}_2(3,2,1/6)$. We…

High Energy Physics - Phenomenology · Physics 2025-01-13 P. S. Bhupal Dev , Srubabati Goswami , Chayan Majumdar , Debashis Pachhar

Collective flavor transformations in supernovae, caused by neutrino-neutrino interactions, are essentially a two-flavor phenomenon driven by the atmospheric mass difference and the small mixing angle theta_13. In the two-flavor…

High Energy Physics - Phenomenology · Physics 2010-04-29 Basudeb Dasgupta , Georg G. Raffelt , Irene Tamborra

We investigate the lepton flavor violation decays, $\tau \to \mu\gamma$, $\tau \to e\gamma$ and $\mu \to e\gamma$, in the framwork of a squential fourth generation model with a heavy fourth neutrino, $\nu'$. Using the recent experimental…

High Energy Physics - Phenomenology · Physics 2007-05-23 Wu-Jun Huo , Tai-Fu Feng

We study the impact of flavour in thermal leptogenesis, including the quantum oscillations of the asymmetries in lepton flavour space. In the Boltzmann equations we find different numerical factors and additional terms which can affect the…

High Energy Physics - Phenomenology · Physics 2009-11-11 A. Abada , S. Davidson , F-X. J. Michaux , M. Losada , A. Riotto

Leptons with essentially the same properties apart from their mass are grouped into three families (or flavours). The number of leptons of each flavour is conserved in interactions, but this is not imposed by fundamental principles. Since…

High Energy Physics - Experiment · Physics 2021-10-05 ATLAS Collaboration

A search for neutrino oscillations induced by Lorentz violation has been performed using 4,438 live-days of Super-Kamiokande atmospheric neutrino data. The Lorentz violation is included in addition to standard three-flavor oscillations…

High Energy Physics - Experiment · Physics 2015-03-18 Kamiokande Collaboration , K. Abe , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , Y. Nakano , S. Nakayama , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , H. Tanaka , T. Tomura , K. Ueno , R. A. Wendell , T. Yokozawa , T. Irvine , T. Kajita , I. Kametani , K. Kaneyuki , K. P. Lee , T. McLachlan , Y. Nishimura , E. Richard , K. Okumura , L. Labarga , P. Fernandez , J. Gustafson , E. Kearns , J. L. Raaf , S. Berkman , H. A. Tanaka , S. Tobayama , J. L. Stone , L. R. Sulak , M. Goldhaber , G. Carminati , W. R. Kropp , S. Mine , P. Weatherly , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , T. Akiri , A. Himmel , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , C. Bronner , S. Hirota , K. Huang , K. Ieki , T. Kikawa , A. Minamino , A. Murakami , T. Nakaya , K. Suzuki , S. Takahashi , K. Tateishi , Y. Fukuda , K. Choi , Y. Itow , G. Mitsuka , P. Mijakowski , J. Hignight , J. Imber , C. K. Jung , C. Yanagisawa , H. Ishino , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , R. Yamaguchi , T. Yano , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Suda , Y. Totsuka , M. Yokoyama , K. Martens , Ll. Marti , M. R. Vagins , J. F. Martin , P. de Perio , A. Konaka , M. J. Wilking , S. Chen , Y. Zhang , K. Connolly , R. J. Wilkes
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