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The number of sigma of confidence in a determination of the neutrino mass hierarchy may be obtained from the statistic Delta chi squared. However, as the hierarchy is a discrete variable, this number is not given by the usual square root…

High Energy Physics - Phenomenology · Physics 2013-11-15 Jarah Evslin

We study the effects of neutrino oscillation on supernova neutrino in the case of the inverted mass hierarchy ($m_{3} \ll m_{1} < m_{2}$) as well as the normal mass hierarchy ($m_{1} < m_{2} \ll m_{3}$). Numerical analysis using a realistic…

High Energy Physics - Phenomenology · Physics 2009-11-07 K. Takahashi , K. Sato

In this work, we explore the possibility of probing the mass ordering sensitivity as a function of supernova distance in the context of the ongoing neutrino experiment NO$\nu$A. We provide a detailed study of the active-active and…

High Energy Physics - Phenomenology · Physics 2025-06-24 Papia Panda , Rukmani Mohanta

The Jiangmen Underground Neutrino Observatory (JUNO) is a large and high precision liquid scintillator detector under construction in the south of China. With its 20 kt target mass, it aims to achieve an unprecedented 3% energy resolution…

Instrumentation and Detectors · Physics 2016-12-19 Marco Grassi

The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed. The data concern different event topologies with average neutrino energies of ~ 4 and ~ 50 GeV. The Multiple Coulomb Scattering of muons…

High Energy Physics - Experiment · Physics 2019-08-14 G. Giacomelli

The final results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed. The data concern different event topologies with average neutrino energies of ~3 and ~50 GeV. Multiple Coulomb Scattering of the…

High Energy Physics - Experiment · Physics 2009-11-10 G. Giacomelli , A. Margiotta

The main goal of the Jiangmen Underground Neutrino Observatory (JUNO) under construction in China is to determine the neutrino mass hierarchy and to measure oscillation parameters to the sub-percent level. The detector consists of 20 ktons…

Instrumentation and Detectors · Physics 2022-05-25 Pierre-Alexandre Petitjean , Barbara Clerbaux , Marta Colomer Molla , Yifan Yang

Neutrino mixing and basics of neutrino oscillations are considered. Recent evidences in favour of neutrino oscillations, obtained in the solar and atmospheric neutrino experiments, are discussed. Neutrino oscillations in the solar and…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. M. Bilenky

RENO (Reactor Experiment for Neutrino Oscillation) is an experiment dedicated to measure the smallest neutrino mixing angle {\theta}_13 using reactor neutrinos in Korea. Our first result measured in 2012 using about 220 live days of data…

Instrumentation and Detectors · Physics 2013-12-18 Seon-Hee Seo

A neutrino-oscillation analysis is performed of the more finely binned Super-K atmospheric, MINOS, and CHOOZ data in order to examine the impact of neutrino hierarchy in this data set upon the value of $\theta_{13}$ and the deviation of…

Nuclear Theory · Physics 2011-06-21 J. Escamilla-Roa , D. C. Latimer , D. J. Ernst

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

RENO (Reactor Experiment for Neutrino Oscillation) has made a definitive measurement of the smallest mixing angle theta13 in 2012, based on the disappearance of electron antineutrinos. More precise measurements have been obtained and…

High Energy Physics - Experiment · Physics 2014-12-11 Soo-Bong Kim

The main goal of the JUNO experiment is to determine the neutrino mass ordering with a 20kt liquid-scintillator detector. The 20-inch PMT and its 1F3 (one for three) electronics are crucial to realize the excellent energy resolution of at…

We present a search for non-zero theta_{13} and deviations of sin^2 theta_{23} from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande -I, -II, and -III. No distortions of the neutrino flux consistent with non-zero…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , R. Wendell , C. Ishihara , K. Abe , Y. Hayato , T. Iida , M. Ikeda , K. Iyogi , J. Kameda , K. Kobayashi , Y. Koshio , Y. Kozuma , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Obayashi , H. Ogawa , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Ueno , K. Ueshima , H. Watanabe , S. Yamada , T. Yokozawa , S. Hazama , H. Kaji , T. Kajita , K. Kaneyuki , T. McLachlan , K. Okumura , Y. Shimizu , N. Tanimoto , M. R. Vagins , F. Dufour , E. Kearns , M. Litos , J. L. Raaf , J. L. Stone , L. R. Sulak , W. Wang , M. Goldhaber , K. Bays , D. Casper , J. P. Cravens , W. R. Kropp , S. Mine , C. Regis , M. B. Smy , H. W. Sobel , K. S. Ganezer , J. Hill , W. E. Keig , J. S. Jang , J. Y. Kim , I. T. Lim , J. Albert , M. Fechner , K. Scholberg , C. W. Walter , S. Tasaka , J. G. Learned , S. Matsuno , Y. Watanabe , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , K. Nishikawa , H. Nishino , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , A. Minamino , T. Nakaya , Y. Fukuda , Y. Itow , G. Mitsuka , T. Tanaka , C. K. Jung , G. Lopez , C. McGrew , C. Yanagisawa , N. Tamura , H. Ishino , A. Kibayashi , S. Mino , T. Mori , M. Sakuda , H. Toyota , Y. Kuno , M. Yoshida , S. B. Kim , B. S. Yang , T. Ishizuka , H. Okazawa , Y. Choi , K. Nishijima , Y. Yokosawa , M. Koshiba , M. Yokoyama , Y. Totsuka , S. Chen , Y. Heng , Z. Yang , H. Zhang , D. Kielczewska , P. Mijakowski , K. Connolly , M. Dziomba , E. Thrane , R. J. Wilkes

We study oscillations of the high energy atmospheric neutrinos in the Earth into sterile neutrinos with the eV-scale mass. The MSW resonance and parametric enhancement of the $\bar{\nu}_\mu\to\bar{\nu}_s$ oscillations lead to distortion of…

High Energy Physics - Phenomenology · Physics 2015-06-16 Arman Esmaili , Alexei Yu. Smirnov

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

Pioneering atmospheric muon neutrino experiments have demonstrated the near-maximal magnitude of the flavor mixing angle $\theta_{23}$. But the precise value of the deviation $D \equiv 1/2 - \sin^2 \theta_{23}$ from maximality (if nonzero)…

High Energy Physics - Phenomenology · Physics 2009-11-11 Sandhya Choubey , Probir Roy

A precise measurement of the atmospheric mass-squared splitting |\Delta m^2_{\mu\mu}| is crucial to establish the three-flavor paradigm and to constrain the neutrino mass models. In addition, a precise value of |\Delta m^2_{\mu\mu}| will…

High Energy Physics - Phenomenology · Physics 2013-12-06 Sanjib Kumar Agarwalla , Suprabh Prakash , Wei Wang

The Jiangmen Underground Neutrino Observatory (JUNO) is proposed to determine the neutrino mass hierarchy using an underground liquid scintillator detector. It is located 53 km away from both Yangjiang and Taishan Nuclear Power Plants in…

Instrumentation and Detectors · Physics 2015-09-29 T. Adam , F. An , G. An , Q. An , N. Anfimov , V. Antonelli , G. Baccolo , M. Baldoncini , E. Baussan , M. Bellato , L. Bezrukov , D. Bick , S. Blyth , S. Boarin , A. Brigatti , T. Brugière , R. Brugnera , M. Buizza Avanzini , J. Busto , A. Cabrera , H. Cai , X. Cai , A. Cammi , D. Cao , G. Cao , J. Cao , J. Chang , Y. Chang , M. Chen , P. Chen , Q. Chen , S. Chen , S. Chen , S. Chen , X. Chen , Y. Chen , Y. Cheng , D. Chiesa , A. Chukanov , M. Clemenza , B. Clerbaux , D. D'Angelo , H. de Kerret , Z. Deng , Z. Deng , X. Ding , Y. Ding , Z. Djurcic , S. Dmitrievsky , M. Dolgareva , D. Dornic , E. Doroshkevich , M. Dracos , O. Drapier , S. Dusini , M. A. Díaz , T. Enqvist , D. Fan , C. Fang , J. Fang , X. Fang , L. Favart , D. Fedoseev , G. Fiorentini , R. Ford , A. Formozov , R. Gaigher , H. Gan , A. Garfagnini , G. Gaudiot , C. Genster , M. Giammarchi , F. Giuliani , M. Gonchar , G. Gong , H. Gong , M. Gonin , Y. Gornushkin , M. Grassi , C. Grewing , V. Gromov , M. Gu , M. Guan , V. Guarino , W. Guo , X. Guo , Y. Guo , M. Göger-Neff , P. Hackspacher , C. Hagner , R. Han , Z. Han , J. Hao , M. He , D. Hellgartner , Y. Heng , D. Hong , S. Hou , Y. Hsiung , B. Hu , J. Hu , S. Hu , T. Hu , W. Hu , H. Huang , X. Huang , X. Huang , L. Huo , W. Huo , A. Ioannisian , D. Ioannisyan , M. Jeitler , K. Jen , S. Jetter , X. Ji , X. Ji , S. Jian , D. Jiang , X. Jiang , C. Jollet , M. Kaiser , B. Kan , L. Kang , M. Karagounis , N. Kazarian , S. Kettell , D. Korablev , A. Krasnoperov , S. Krokhaleva , Z. Krumshteyn , A. Kruth , P. Kuusiniemi , T. Lachenmaier , L. Lei , R. Lei , X. Lei , R. Leitner , F. Lenz , C. Li , F. Li , F. Li , J. Li , N. Li , S. Li , T. Li , W. Li , W. Li , X. Li , X. Li , X. Li , X. Li , Y. Li , Y. Li , Z. Li , H. Liang , H. Liang , J. Liang , M. Licciardi , G. Lin , S. Lin , T. Lin , Y. Lin , I. Lippi , G. Liu , H. Liu , H. Liu , J. Liu , J. Liu , J. Liu , J. Liu , Q. Liu , Q. Liu , S. Liu , S. Liu , Y. Liu , P. Lombardi , Y. Long , S. Lorenz , C. Lu , F. Lu , H. Lu , J. Lu , J. Lu , J. Lu , B. Lubsandorzhiev , S. Lubsandorzhiev , L. Ludhova , F. Luo , S. Luo , Z. Lv , V. Lyashuk , Q. Ma , S. Ma , X. Ma , X. Ma , Y. Malyshkin , F. Mantovani , Y. Mao , S. Mari , D. Mayilyan , W. McDonough , G. Meng , A. Meregaglia , E. Meroni , M. Mezzetto , J. Min , L. Miramonti , M. Montuschi , N. Morozov , T. Mueller , P. Muralidharan , M. Nastasi , D. Naumov , E. Naumova , I. Nemchenok , Z. Ning , H. Nunokawa , L. Oberauer , J. P. Ochoa-Ricoux , A. Olshevskiy , F. Ortica , H. Pan , A. Paoloni , N. Parkalian , S. Parmeggiano , V. Pec , N. Pelliccia , H. Peng , P. Poussot , S. Pozzi , E. Previtali , S. Prummer , F. Qi , M. Qi , S. Qian , X. Qian , H. Qiao , Z. Qin , G. Ranucci , A. Re , B. Ren , J. Ren , T. Rezinko , B. Ricci , M. Robens , A. Romani , B. Roskovec , X. Ruan , X. Ruan , A. Rybnikov , A. Sadovsky , P. Saggese , G. Salamanna , J. Sawatzki , J. Schuler , A. Selyunin , G. Shi , J. Shi , Y. Shi , V. Sinev , C. Sirignano , M. Sisti , O. Smirnov , M. Soiron , A. Stahl , L. Stanco , J. Steinmann , V. Strati , G. Sun , X. Sun , Y. Sun , Y. Sun , D. Taichenachev , J. Tang , A. Tietzsch , I. Tkachev , W. H. Trzaska , Y. Tung , S. van Waasen , C. Volpe , V. Vorobel , L. Votano , C. Wang , C. Wang , C. Wang , G. Wang , H. Wang , M. Wang , R. Wang , S. Wang , W. Wang , W. Wang , Y. Wang , Y. Wang , Y. Wang , Y. Wang , Z. Wang , Z. Wang , Z. Wang , Z. Wang , Z. Wang , W. Wei , Y. Wei , M. Weifels , L. Wen , Y. Wen , C. Wiebusch , S. Wipperfurth , S. C. Wong , B. Wonsak , C. Wu , Q. Wu , Z. Wu , M. Wurm , J. Wurtz , Y. Xi , D. Xia , J. Xia , M. Xiao , Y. Xie , J. Xu , J. Xu , L. Xu , Y. Xu , B. Yan , X. Yan , C. Yang , C. Yang , H. Yang , L. Yang , M. Yang , Y. Yang , Y. Yang , Y. Yang , E. Yanovich , Y. Yao , M. Ye , X. Ye , U. Yegin , F. Yermia , Z. You , B. Yu , C. Yu , C. Yu , G. Yu , Z. Yu , Y. Yuan , Z. Yuan , M. Zanetti , P. Zeng , S. Zeng , T. Zeng , L. Zhan , C. Zhang , F. Zhang , G. Zhang , H. Zhang , J. Zhang , J. Zhang , J. Zhang , K. Zhang , P. Zhang , Q. Zhang , T. Zhang , X. Zhang , X. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Z. Zhang , Z. Zhang , J. Zhao , M. Zhao , T. Zhao , Y. Zhao , H. Zheng , M. Zheng , X. Zheng , Y. Zheng , W. Zhong , G. Zhou , J. Zhou , L. Zhou , N. Zhou , R. Zhou , S. Zhou , W. Zhou , X. Zhou , Y. Zhou , H. Zhu , K. Zhu , H. Zhuang , L. Zong , J. Zou

We investigate the potential of the next generation long-baseline neutrino experiments DUNE and T2HK as well as the upcoming reactor experiment JUNO to constrain Non-Standard Interaction (NSI) parameters. JUNO is going to provide the most…

High Energy Physics - Phenomenology · Physics 2021-04-14 Pouya Bakhti , Meshkat Rajaee