English
Related papers

Related papers: Model Predictions for Neutrino Oscillation Paramet…

200 papers

A new type of neutrino mixing named bi-pair neutrino mixing is proposed to describe the current neutrino mixing pattern with a vanishing reactor mixing angle and is determined by a mixing matrix with two pairs of identical magnitudes of…

High Energy Physics - Phenomenology · Physics 2011-02-11 Teruyuki Kitabayashi , Masaki Yasue

We present updated values for the mass-mixing parameters relevant to neutrino oscillations, with particular attention to emerging hints in favor of theta_13>0. We also discuss the status of absolute neutrino mass observables, and a possible…

High Energy Physics - Phenomenology · Physics 2008-09-19 G. L. Fogli , E. Lisi , A. Marrone , A. Palazzo , A. M. Rotunno

We show that in a reactor disappearance oscillation experiment the sensitivity to the mixing parameter can be substantially improved for $(1 - 5\cdot10^{-4}) eV^{2}$ mass parameter range which includes both the LSND and the atmospheric…

High Energy Physics - Phenomenology · Physics 2011-04-15 L. A. Mikaelyan , V. V. Sinev

The next generation of double-beta decay experiments have an excellent chance of providing data on the neutrino mass pattern. This presentation is a summary of what is currently known about the mass pattern and expectations from experiment.…

Nuclear Experiment · Physics 2015-06-26 Steven R. Elliott

We review the present understanding of neutrino masses and mixings, discussing what are the unknowns in the three family oscillation scenario. Despite the anticipated success coming from the planned long baseline neutrino experiments in…

High Energy Physics - Phenomenology · Physics 2009-11-11 Olga Mena

In view of the recently reported evidence for a nonzero Majorana mass of the electron neutrino, together with the established phenomena of atmospheric and solar neutrino oscillations, the case of three nearly mass-degenerate Majorana…

High Energy Physics - Phenomenology · Physics 2009-11-07 Ernest Ma

Neutrino oscillations reveal several small parameters, namely, $\theta_{13}$, the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one, and the deviation of $\theta_{23}$ from maximal mixing. Can these small quantities all be traced…

High Energy Physics - Phenomenology · Physics 2015-05-27 Soumita Pramanick , Amitava Raychaudhuri

Neutrino oscillations are studied employing sources of low energy monoenergetic neutrinos following electron capture by the nucleus and measuring electron recoils. Since the neutrino energy is very low the oscillation length appearing in…

High Energy Physics - Phenomenology · Physics 2011-01-27 J. D. Vergados , Y. Giomataris , Yu. N. Novikov

The tetra-maximal neutrino mixing pattern predicts a relatively large reactor mixing angle theta_13 \approx 8.4^\circ, which is in good agreement with the latest best-fit value theta_13 = 9^\circ. However, its prediction for theta_12…

High Energy Physics - Phenomenology · Physics 2015-05-28 He Zhang , Shun Zhou

Here we update our previous global fit of neutrino oscillations by including the recent results which have appeared since the Neutrino-2012 conference. These include the measurements of reactor anti-neutrino disappearance reported by Daya…

High Energy Physics - Phenomenology · Physics 2014-11-26 D. V. Forero , M. Tortola , J. W. F. Valle

One of the main goals of RENO (Reactor Experiment for Neutrino Oscillation) is to measure the smallest neutrino mixing angle {\theta}13 using reactor neutrinos in Korea. RENO is the first reactor experiment taking data with two identical…

High Energy Physics - Experiment · Physics 2019-08-21 Seon-Hee Seo

Any new neutrino physics at the TeV scale must include a suppression mechanism to keep its contribution to light neutrino masses small enough. We review some seesaw model examples with weakly broken lepton number, and comment on the…

High Energy Physics - Phenomenology · Physics 2008-11-26 F. del Aguila , J. A. Aguilar Saavedra , J. de Blas , M. Zralek

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

We performed a simulation on the DUNE experiment to probe the capability of future neutrino long-baseline experiments' ability to constrain the parameter space of high-energy models by using the correlation between the atmospheric and…

High Energy Physics - Phenomenology · Physics 2017-11-29 Pedro Pasquini

We perform an updated global analysis of the known and unknown parameters of the standard $3\nu$ framework as of 2025. The known oscillation parameters include three mixing angles $(\theta_{12},\,\theta_{23},\,\theta_{13})$ and two squared…

High Energy Physics - Phenomenology · Physics 2025-03-12 Francesco Capozzi , William Giarè , Eligio Lisi , Antonio Marrone , Alessandro Melchiorri , Antonio Palazzo

The Cervera et al. formula, the best known approximate formula of neutrino oscillation probability for long-baseline experiments, can be regarded as a second-order perturbative formula with small expansion parameter epsilon \equiv Delta…

High Energy Physics - Phenomenology · Physics 2015-03-19 Katsuhiro Asano , Hisakazu Minakata

The T2K experiment observes indications of $\nu_\mu\rightarrow \nu_e$ appearance in data accumulated with $1.43\times10^{20}$ protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino…

High Energy Physics - Experiment · Physics 2011-08-01 T2K Collaboration , K. Abe , N. Abgrall , Y. Ajima , H. Aihara , J. B. Albert , C. Andreopoulos , B. Andrieu , S. Aoki , O. Araoka , J. Argyriades , A. Ariga , T. Ariga , S. Assylbekov , D. Autiero , A. Badertscher , M. Barbi , G. J. Barker , G. Barr , M. Bass , F. Bay , S. Bentham , V. Berardi , B. E. Berger , I. Bertram , M. Besnier , J. Beucher , D. Beznosko , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , C. Bojechko , J. Bouchez , S. B. Boyd , A. Bravar , C. Bronner , D. G. Brook-Roberge , N. Buchanan , H. Budd , D. Calvet , S. L. Cartwright , A. Carver , R. Castillo , M. G. Catanesi , A. Cazes , A. Cervera , C. Chavez , S. Choi , G. Christodoulou , J. Coleman , W. Coleman , G. Collazuol , K. Connolly , A. Curioni , A. Dabrowska , I. Danko , R. Das , G. S. Davies , S. Davis , M. Day , G. DeRosa , J. P. A. M. de Andre , P. dePerio , A. Delbart , C. Densham , F. DiLodovico , S. DiLuise , P. Dinh Tran , J. Dobson , U. Dore , O. Drapier , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , M. Dziomba , S. Emery , A. Ereditato , L. Escudero , L. S. Esposito , M. Fechner , A. Ferrero , A. J. Finch , E. Frank , Y. Fujii , Y. Fukuda , V. Galymov , F. C. Gannaway , A. Gaudin , A. Gendotti , M. George , S. Giffin , C. Giganti , K. Gilje , T. Golan , M. Goldhaber , J. J. Gomez-Cadenas , M. Gonin , N. Grant , A. Grant , P. Gumplinger , P. Guzowski , A. Haesler , M. D. Haigh , K. Hamano , C. Hansen , D. Hansen , T. Hara , P. F. Harrison , B. Hartfiel , M. Hartz , T. Haruyama , T. Hasegawa , N. C. Hastings , S. Hastings , A. Hatzikoutelis , K. Hayashi , Y. Hayato , C. Hearty , R. L. Helmer , R. Henderson , N. Higashi , J. Hignight , E. Hirose , J. Holeczek , S. Horikawa , A. Hyndman , A. K. Ichikawa , K. Ieki , M. Ieva , M. Iida , M. Ikeda , J. Ilic , J. Imber , T. Ishida , C. Ishihara , T. Ishii , S. J. Ives , M. Iwasaki , K. Iyogi , A. Izmaylov , B. Jamieson , R. A. Johnson , K. K. Joo , G. V. Jover-Manas , C. K. Jung , H. Kaji , T. Kajita , H. Kakuno , J. Kameda , K. Kaneyuki , D. Karlen , K. Kasami , I. Kato , E. Kearns , M. Khabibullin , F. Khanam , A. Khotjantsev , D. Kielczewska , T. Kikawa , J. Kim , J. Y. Kim , S. B. Kim , N. Kimura , B. Kirby , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , S. Koike , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , Y. Kouzuma , K. Kowalik , V. Kravtsov , I. Kreslo , W. Kropp , H. Kubo , Y. Kudenko , N. Kulkarni , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , M. Laveder , K. P. Lee , P. T. Le , J. M. Levy , C. Licciardi , I. T. Lim , T. Lindner , R. P. Litchfield , M. Litos , A. Longhin , G. D. Lopez , P. F. Loverre , L. Ludovici , T. Lux , M. Macaire , K. Mahn , Y. Makida , M. Malek , S. Manly , A. Marchionni , A. D. Marino , J. Marteau , J. F. Martin , T. Maruyama , T. Maryon , J. Marzec , P. Masliah , E. L. Mathie , C. Matsumura , K. Matsuoka , V. Matveev , K. Mavrokoridis , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , T. McLachlan , M. Messina , W. Metcalf , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , S. Mine , A. D. Missert , G. Mituka , M. Miura , K. Mizouchi , L. Monfregola , F. Moreau , B. Morgan , S. Moriyama , A. Muir , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nakadaira , M. Nakahata , T. Nakai , K. Nakajima , T. Nakamoto , K. Nakamura , S. Nakayama , T. Nakaya , D. Naples , M. L. Navin , B. Nelson , T. C. Nicholls , K. Nishikawa , H. Nishino , J. A. Nowak , M. Noy , Y. Obayashi , T. Ogitsu , H. Ohhata , T. Okamura , K. Okumura , T. Okusawa , S. M. Oser , M. Otani , R. A. Owen , Y. Oyama , T. Ozaki , M. Y. Pac , V. Palladino , V. Paolone , P. Paul , D. Payne , G. F. Pearce , J. D. Perkin , V. Pettinacci , F. Pierre , E. Poplawska , B. Popov , M. Posiadala , J. -M. Poutissou , R. Poutissou , P. Przewlocki , W. Qian , J. L. Raaf , E. Radicioni , P. N. Ratoff , T. M. Raufer , M. Ravonel , M. Raymond , F. Retiere , A. Robert , P. A. Rodrigues , E. Rondio , J. M. Roney , B. Rossi , S. Roth , A. Rubbia , D. Ruterbories , S. Sabouri , R. Sacco , K. Sakashita , F. Sanchez , A. Sarrat , K. Sasaki , K. Scholberg , J. Schwehr , M. Scott , D. I. Scully , Y. Seiya , T. Sekiguchi , H. Sekiya , M. Shibata , Y. Shimizu , M. Shiozawa , S. Short , M. Syiad , R. J. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , A. Stahl , P. Stamoulis , J. Steinmann , B. Still , J. Stone , C. Strabel , L. R. Sulak , R. Sulej , P. Sutcliffe , A. Suzuki , K. Suzuki , S. Suzuki , S. Y. Suzuki , Y. Suzuki , Y. Suzuki , T. Szeglowski , M. Szeptycka , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Tanaka , H. A. Tanaka , M. Tanaka , M. M. Tanaka , N. Tanimoto , K. Tashiro , I. Taylor , A. Terashima , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , W. Toki , T. Tomaru , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , K. Ueno , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , J. J. Walding , A. V. Waldron , C. W. Walter , P. J. Wanderer , J. Wang , M. A. Ward , G. P. Ward , D. Wark , M. O. Wascko , A. Weber , R. Wendell , N. West , L. H. Whitehead , G. Wikstrom , R. J. Wilkes , M. J. Wilking , J. R. Wilson , R. J. Wilson , T. Wongjirad , S. Yamada , Y. Yamada , A. Yamamoto , K. Yamamoto , Y. Yamanoi , H. Yamaoka , C. Yanagisawa , T. Yano , S. Yen , N. Yershov , M. Yokoyama , A. Zalewska , J. Zalipska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

Recent data in the neutrino sector point towards a relatively large value of the reactor angle, incompatible with a vanishing theta_ 13 at about 3 sigma. In order to explain such a result, we propose a SUSY model based on the broken…

High Energy Physics - Phenomenology · Physics 2015-05-30 Davide Meloni

A model of neutrino oscillations is presented that has only three degrees of freedom and is consistent with existing data. The model is a subset of the renormalizable sector of the Standard-Model Extension (SME), and it offers an…

High Energy Physics - Phenomenology · Physics 2008-11-26 Teppei Katori , Alan Kostelecky , Rex Tayloe

The discovery of neutrino mass establishes the need for physics beyond the Standard Model. I summarize the status of two- and three-neutrino oscillation parameters from current solar, atmospheric, reactor and accelerator data. Future…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. W. F. Valle