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Related papers: Understanding the degeneracies in NO$\nu$A data

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We examine the use of two superbeam neutrino oscillation experiments with baselines $\lsim 1000$ km to resolve parameter degeneracies inherent in the three-neutrino analysis of such experiments. We find that with appropriate choices of…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , D. Marfatia , K. Whisnant

Current 3$\nu$ global fits predict two degenerate solutions for $\theta_{23}$: one lies in lower octant ($\theta_{23} <\pi/4$), and the other belongs to higher octant ($\theta_{23} >\pi/4$). Here, we study how the measurement of…

High Energy Physics - Phenomenology · Physics 2017-04-25 Sanjib Kumar Agarwalla , Sabya Sachi Chatterjee , Antonio Palazzo

We suggest mass matrices for neutrinos and charged leptons that can explain solar and atmospheric neutrino data. The resulting flavor mixing matrix $V_{\nu}$ has a property that $(V_{\nu})_{13}=0$, thus making $\nu_e \leftrightarrow…

High Energy Physics - Phenomenology · Physics 2009-10-30 Kyungsik Kang , Sin Kyu Kang , Jihn E. Kim , Pyungwon Ko

The two long-baseline experiments ICARUS and OPERA have recently provided bounds on light ($\sim$ eV) sterile neutrinos exploiting the negative results of the $\nu_\mu \to \nu_e$ appearance searches. Both collaborations have performed the…

High Energy Physics - Phenomenology · Physics 2015-06-11 Antonio Palazzo

Neutrino non-standard interactions (NSI) with the first generation of standard model fermions can span a parameter space of large dimension and exhibit degeneracies that cannot be broken by a single class of experiment. Oscillation…

High Energy Physics - Phenomenology · Physics 2020-09-22 Bhaskar Dutta , Rafael F. Lang , Shu Liao , Samiran Sinha , Louis Strigari , Adrian Thompson

I discuss in this talk mainly three topics related with dark matter motivated neutrino mass spectrum and a generic issue of mass pattern, the normal versus the inverted mass hierarchies. In the first part, by describing failure of a…

High Energy Physics - Phenomenology · Physics 2007-05-23 Hisakazu Minakata

The presence of degeneracies can considerably worsen the measure of the neutrino oscillation parameters $\theta_{13}$ and $\delta$. We study the physics reach of a specific ``CERN'' setup, using a standard $\beta$-Beam and Super-Beam…

High Energy Physics - Phenomenology · Physics 2014-11-18 S. Rigolin

The recent data indicate that the neutrino mixing angle $\theta_{23}$ deviates from the maximal-mixing value of 45$^\circ$, showing two nearly degenerate solutions, one in the lower octant (LO) ($\theta_{23}<45^\circ$) and one in the higher…

High Energy Physics - Phenomenology · Physics 2018-03-02 C. R. Das , Jukka Maalampi , João Pulido , Sampsa Vihonen

Sterile neutrinos are one candidate to explain anomalies in neutrino oscillations. The mass-difference-driving oscillation between flavors can be probed only within specific combinations of baseline and flight energy. For a neutrino whose…

High Energy Physics - Phenomenology · Physics 2013-03-26 S. K. Kang , Y. D. Kim , Y. Ko , K. Siyeon

This Letter reports a search for charge-parity ($CP$) symmetry violating nonstandard interactions (NSI) of neutrinos with matter using the NOvA Experiment, and examines their effects on the determination of the standard oscillation…

High Energy Physics - Experiment · Physics 2024-11-28 NOvA Collaboration , M. A. Acero , B. Acharya , P. Adamson , L. Aliaga , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , N. Balashov , P. Baldi , B. A. Bambah , A. Bat , K. Bays , R. Bernstein , T. J. C. Bezerra , V. Bhatnagar , D. Bhattarai , B. Bhuyan , J. Bian , A. C. Booth , R. Bowles , B. Brahma , C. Bromberg , N. Buchanan , A. Butkevich , S. Calvez , T. J. Carroll , E. Catano-Mur , J. P. Cesar , A. Chatla , S. Chaudhary , R. Chirco , B. C. Choudhary , A. Christensen , M. F. Cicala , T. E. Coan , A. Cooleybeck , C. Cortes-Parra , D. Coveyou , L. Cremonesi , G. S. Davies , P. F. Derwent , Z. Djurcic , M. Dolce , D. Doyle , D. Dueñas Tonguino , E. C. Dukes , A. Dye , R. Ehrlich , E. Ewart , P. Filip , J. Franc , M. J. Frank , H. R. Gallagher , F. Gao , A. Giri , R. A. Gomes , M. C. Goodman , M. Groh , R. Group , A. Habig , F. Hakl , J. Hartnell , R. Hatcher , M. He , K. Heller , V Hewes , A. Himmel , Y. Ivaneev , A. Ivanova , B. Jargowsky , J. Jarosz , C. Johnson , M. Judah , I. Kakorin , D. M. Kaplan , A. Kalitkina , J. Kleykamp , O. Klimov , L. W. Koerner , L. Kolupaeva , R. Kralik , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , J. Lesmeister , A. Lister , J. Liu , J. A. Lock , M. Lokajicek , M. MacMahon , S. Magill , W. A. Mann , M. T. Manoharan , M. Manrique Plata , M. L. Marshak , M. Martinez-Casales , V. Matveev , B. Mehta , M. D. Messier , H. Meyer , T. Miao , V. Mikola , W. H. Miller , S. Mishra , S. R. Mishra , A. Mislivec , R. Mohanta , A. Moren , A. Morozova , W. Mu , L. Mualem , M. Muether , K. Mulder , D. Myers , D. Naples , A. Nath , S. Nelleri , J. K. Nelson , R. Nichol , E. Niner , A. Norman , A. Norrick , T. Nosek , H. Oh , A. Olshevskiy , T. Olson , M. Ozkaynak , A. Pal , J. Paley , L. Panda , R. B. Patterson , G. Pawloski , O. Petrova , R. Petti , L. R. Prais , A. Rafique , V. Raj , M. Rajaoalisoa , B. Ramson , M. Ravelhofer , B. Rebel , P. Roy , O. Samoylov , M. C. Sanchez , S. Sánchez Falero , P. Shanahan , P. Sharma , A. Shmakov , A. Sheshukov , S. Shukla , D. K. Singha , W. Shorrock , I. Singh , P. Singh , V. Singh , E. Smith , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , L. Suter , A. Sutton , K. Sutton , S. Swain , C. Sweeney , A. Sztuc , B. Tapia Oregui , P. Tas , T. Thakore , J. Thomas , E. Tiras , Y. Torun , J. Tripathi , J. Trokan-Tenorio , J. Urheim , P. Vahle , Z. Vallari , J. Vasel , J. D. Villamil , K. J. Vockerodt , T. Vrba , M. Wallbank , M. Wetstein , D. Whittington , D. A. Wickremasinghe , T. Wieber , J. Wolcott , M. Wrobel , S. Wu , W. Wu , Y. Xiao , B. Yaeggy , A. Yahaya , A. Yankelevich , K. Yonehara , Y. Yu , S. Zadorozhnyy , J. Zalesak , R. Zwaska

Present global fits of world neutrino data hint towards non-maximal $\theta_{23}$ with two nearly degenerate solutions, one in the lower octant ($\theta_{23} <\pi/4$), and the other in the higher octant ($\theta_{23} >\pi/4$). This octant…

High Energy Physics - Phenomenology · Physics 2017-01-25 Sanjib Kumar Agarwalla , Sabya Sachi Chatterjee , Antonio Palazzo

We study neutrino oscillation within the framework of three generations in matter. We propose a simple method to approximate the coefficients A, B and C which do not depend on the CP phase \delta in the oscillation probability P(\nu_e \to…

High Energy Physics - Phenomenology · Physics 2014-11-17 Akira Takamura , Keiichi Kimura , Hidekazu Yokomakura

Neutrino mass hierarchy, CP-violation, and octant of $\theta_{23}$ are the fundamental unknowns in neutrino oscillations. In order to address all these three unknowns, we study the physics reach of a setup, where we replace the antineutrino…

High Energy Physics - Phenomenology · Physics 2017-08-23 Sanjib Kumar Agarwalla , Monojit Ghosh , Sushant K. Raut

We have previously shown that the decay of high-energy neutrinos from distant astrophysical sources would be revealed by flavor ratios that deviate strongly from the $\phi_{\nu_e}:\phi_{\nu_\mu}:\phi_{\nu_\tau} = 1:1:1$ expected from…

High Energy Physics - Phenomenology · Physics 2008-11-26 John F. Beacom , Nicole F. Bell , Dan Hooper , Sandip Pakvasa , Thomas J. Weiler

We discuss various physics aspects of neutrino oscillation with non-standard interactions (NSI). We formulate a perturbative framework by taking \Delta m^2_{21} / \Delta m^2_{31}, s_{13}, and the NSI elements \epsilon_{\alpha \beta}…

High Energy Physics - Phenomenology · Physics 2009-03-27 Takashi Kikuchi , Hisakazu Minakata , Shoichi Uchinami

The OPERA experiment was designed to study $\nu_\mu\to\nu_\tau$ oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to…

High Energy Physics - Experiment · Physics 2018-05-30 OPERA Collaboration , N. Agafonova , A. Alexandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , A. Bertolin , C. Bozza , R. Brugnera , A. Buonaura , S. Buontempo , M. Chernyavskiy , A. Chukanov , L. Consiglio , N. D'Ambrosio , G. De Lellis , M. De Serio , P. del Amo Sanchez , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievsky , M. Dracos , D. Duchesneau , S. Dusini , T. Dzhatdoev , J. Ebert , A. Ereditato , J. Favier , R. A. Fini , F. Fornari , T. Fukuda , G. Galati , A. Garfagnini , V. Gentile , J. Goldberg , Y. Gornushkin , S. Gorbunov , G. Grella , A. M. Guler , C. Gustavino , C. Hagner , T. Hara , T. Hayakawa , A. Hollnagel , K. Ishiguro , A. Iuliano , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , S. H. Kim , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , F. Laudisio , A. Lauria , A. Ljubicic , A. Longhin , P. Loverre , A. Malgin , M. Malenica , G. Mandrioli , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , S. Mikado , M. Miyanishi , F. Mizutani , P. Monacelli , M. C. Montesi , K. Morishima , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , K. Niwa , N. Okateva , A. Olchevsky , S. Ogawa , K. Ozaki , A. Paoloni , L. Paparella , B. D. Park , L. Pasqualini , A. Pastore , L. Patrizii , H. Pessard , C. Pistillo , D. Podgrudkov , N. Polukhina , M. Pozzato , F. Pupilli , M. Roda , T. Roganova , H. Rokujo , G. Rosa , O. Ryazhskaya , A. Sadovsky , O. Sato , A. Schembri , I. Shakiryanova , T. Shchedrina , H. Shibuya , E. Shibayama , T. Shiraishi , S. Simone , C. Sirignano , G. Sirri , A. Sotnikov , M. Spinetti , L. Stanco , N. Starkov , S. M. Stellacci , M. Stipcevic , P. Strolin , S. Takahashi , M. Tenti , F. Terranova , V. Tioukov , S. Tufanli , A. Ustyuzhanin , S. Vasina , P. Vilain , E. Voevodina , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , C. S. Yoon

In this work we present a scenario in which a nonstandard interaction in neutrino propagation can explain the three major tensions in the neutrino oscillation data at present. These tensions are: (i) a non-zero best-fit value of the…

High Energy Physics - Phenomenology · Physics 2016-09-15 Shinya Fukasawa , Monojit Ghosh , Osamu Yasuda

We revisit our previous work [Phys. Rev. D 95, 096014 (2017)] where neutrino oscillation and nonoscillation data were analyzed in the standard framework with three neutrino families, in order to constrain their absolute masses and to probe…

High Energy Physics - Phenomenology · Physics 2020-07-01 Francesco Capozzi , Eleonora Di Valentino , Eligio Lisi , Antonio Marrone , Alessandro Melchiorri , Antonio Palazzo

As the increasing of neutrino energy or matter density, the neutrino oscillation in matter may undergo "vacuum-dominated", "resonance" and "matter-dominated" three different stages successively. Neutrinos endure very different matter…

High Energy Physics - Phenomenology · Physics 2020-02-26 Shu Luo

In this work we analyze quantum decoherence in neutrino oscillations considering the Open Quantum System framework and oscillations through matter for three neutrino families. Taking DUNE as a case study we performed sensitivity analyses…

High Energy Physics - Phenomenology · Physics 2019-09-25 G. Balieiro Gomes , D. V. Forero , M. M. Guzzo , P. C. de Holanda , R. L. N. Oliveira
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