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The recent results from the JUNO reactor neutrino experiment have significantly improved our knowledge of the solar mixing angle $\theta_{12}$ and the solar mass splitting $\Delta m^2_{21}$. We study the impact of these improved estimates…

High Energy Physics - Phenomenology · Physics 2026-01-21 Debasish Borah , Pritam Das , Debajyoti Dutta

To maximize the light yield of the liquid scintillator (LS) for the Jiangmen Underground Neutrino Observatory (JUNO), a 20 t LS sample was produced in a pilot plant at Daya Bay. The optical properties of the new LS in various compositions…

Instrumentation and Detectors · Physics 2020-07-02 Daya Bay , JUNO collaborations , : , A. Abusleme , T. Adam , S. Ahmad , S. Aiello , M. Akram , N. Ali , F. P. An , G. P. An , Q. An , G. Andronico , N. Anfimov , V. Antonelli , T. Antoshkina , B. Asavapibhop , J. P. A. M. de André , A. Babic , A. B. Balantekin , W. Baldini , M. Baldoncini , H. R. Band , A. Barresi , E. Baussan , M. Bellato , E. Bernieri , D. Biare , T. Birkenfeld , M. Bishai , S. Blin , D. Blum , S. Blyth , C. Bordereau , A. Brigatti , R. Brugnera , A. Budano , P. Burgbacher , M. Buscemi , S. Bussino , J. Busto , I. Butorov , A. Cabrera , H. Cai , X. Cai , Y. K. Cai , Z. Y. Cai , A. Cammi , A. Campeny , C. Y. Cao , G. F. Cao , J. Cao , R. Caruso , C. Cerna , I. Chakaberia , J. F. Chang , Y. Chang , H. S. Chen , P. A. Chen , P. P. Chen , S. M. Chen , S. J. Chen , X. R. Chen , Y. W. Chen , Y. X. Chen , Y. Chen , Z. Chen , J. Cheng , Y. P. Cheng , Z. K. Cheng , A. Chepurnov , J. J. Cherwinka , F. Chiarello , D. Chiesa , P. Chimenti , M. C. Chu , A. Chukanov , A. Chuvashova , . Clementi , B. Clerbaux , S. Conforti Di Lorenzo , D. Corti , S. Costa , F. D. Corso , J. P. Cummings , O. Dalager , C. De La Taille , F. S. Deng , J. W. Deng , Z. Deng , Z. Y. Deng , W. Depnering , M. Diaz , X. F. Ding , Y. Y. Ding , B. Dirgantara , S. Dmitrievsky , M. V. Diwan , T. Dohnal , G. Donchenko , J. M. Dong , D. Dornic , E. Doroshkevich , J. Dove , M. Dracos , F. Druillole , S. X. Du , S. Dusini , M. Dvorak , D. A. Dwyer , T. Enqvist , H. Enzmann , A. Fabbri , L. Fajt , D. H. Fan , L. Fan , C. Fang , J. Fang , A. Fatkina , D. Fedoseev , V. Fekete , L. C. Feng , Q. C. Feng , G. Fiorentini , R. Ford , A. Formozov , A. Fournier , S. Franke , J. P. Gallo , H. N. Gan , F. Gao , A. Garfagnini , A. Göttel , C. Genster , M. Giammarchi , A. Giaz , N. Giudice , F. Giuliani , M. Gonchar , G. H. Gong , H. Gong , O. Gorchakov , Y. Gornushkin , M. Grassi , C. Grewing , M. Gromov , V. Gromov , M. H. Gu , W. Q. Gu , X. F. Gu , Y. Gu , M. Y. Guan , N. Guardone , M. Gul , C. Guo , J. Y. Guo , L. Guo , W. L. Guo , X. H. Guo , Y. H. Guo , Z. Guo , M. Haacke , R. W. Hackenburg , P. Hackspacher , C. Hagner , R. Han , Y. Han , S. Hans , M. He , W. He , K. M. Heeger , T. Heinz , Y. K. Heng , R. Herrera , A. Higuera , D. J. Hong , Y. K. Hor , S. J. Hou , Y. B. Hsiung , B. Z. Hu , H. Hu , J. R. Hu , J. Hu , S. Y. Hu , T. Hu , Z. J. Hu , C. H. Huang , G. H. Huang , H. X. Huang , Q. H. Huang , W. H. Huang , X. T. Huang , Y. B. Huang , P. Huber , J. Q. Hui , L. Huo , W. J. Huo , C. Huss , S. Hussain , A. Insolia , A. Ioannisian , D. Ioannisyan , R. Isocrate , D. E. Jaffe , K. L. Jen , X. L. Ji , X. P. Ji , X. Z. Ji , H. H. Jia , J. J. Jia , S. Y. Jian , D. Jiang , X. S. Jiang , R. Y. Jin , X. P. Jing , R. A. Johnson , C. Jollet , D. Jones , J. Joutsenvaara , S. Jungthawan , L. Kalousis , P. Kampmann , L. Kang , M. Karagounis , N. Kazarian , S. H. Kettell , A. Khan , W. Khan , K. Khosonthongkee , P. Kinz , S. Kohn , D. Korablev , K. Kouzakov , M. Kramer , A. Krasnoperov , S. Krokhaleva , Z. Krumshteyn , A. Kruth , N. Kutovskiy , P. Kuusiniemi , B. Lachacinski , T. Lachenmaier , T. J. Langford , J. Lee , J. H. C. Lee , F. Lefevre , L. Lei , R. Lei , R. Leitner , J. Leung , C. Li , D. M. Li , F. Li , F. Li , H. T. Li , H. L. Li , J. Li , J. J. Li , J. Q. Li , K. J. Li , M. Z. Li , N. Li , N. Li , Q. J. Li , Q. J. Li , R. H. Li , S. C. Li , S. F. Li , S. J. Li , T. Li , T. Li , W. D. Li , W. G. Li , X. M. Li , X. N. Li , X. L. Li , X. Q. Li , Y. Li , Y. F. Li , Z. B. Li , Z. Y. Li , H. Liang , H. Liang , J. J. Liang , D. Liebau , A. Limphirat , S. Limpijumnong , C. J. Lin , G. L. Lin , S. X. Lin , T. Lin , Y. H. Lin , J. J. Ling , J. M. Link , I. Lippi , L. Littenberg , B. R. Littlejohn , F. Liu , H. Liu , H. Liu , H. B. Liu , H. D. Liu , H. J. Liu , H. T. Liu , J. C. Liu , J. L. Liu , M. Liu , Q. Liu , Q. Liu , R. X. Liu , S. Y. Liu , S. B. Liu , S. L. Liu , X. W. Liu , Y. Liu , A. Lokhov , P. Lombardi , K. Loo , S. Lorenz , C. Lu , C. Lu , H. Q. Lu , J. B. Lu , J. G. Lu , S. X. Lu , X. X. Lu , B. Lubsandorzhiev , S. Lubsandorzhiev , L. Ludhova , K. B. Luk , F. J. Luo , G. Luo , P. W. Luo , S. Luo , W. M. Luo , V. Lyashuk , Q. M. Ma , S. Ma , X. B. Ma , X. Y. Ma , Y. Q. Ma , Y. Malyshkin , F. Mantovani , Y. J. Mao , S. M. Mari , F. Marini , S. Marium , C. Marshall , C. Martellini , G. Martin-Chassard , D. A. Martinez Caicedo , A. Martini , J. Martino , D. Mayilyan , K. T. McDonald , R. D. McKeown , A. Müller , G. Meng , Y. Meng , A. Meregaglia , E. Meroni , D. Meyhöfer , M. Mezzetto , J. Miller , L. Miramonti , S. Monforte , P. Montini , M. Montuschi , N. Morozov , P. Muralidharan , J. Napolitano , M. Nastasi , D. V. Naumov , E. Naumova , I. Nemchenok , A. Nikolaev , F. P. Ning , Z. Ning , H. Nunokawa , L. Oberauer , J. P. Ochoa-Ricoux , A. Olshevskiy , F. Ortica , H. R. Pan , A. Paoloni , J. Park , N. Parkalian , S. Parmeggiano , S. Patton , T. Payupol , V. Pec , D. Pedretti , Y. T. Pei , N. Pelliccia , A. G. Peng , H. P. Peng , J. C. Peng , F. Perrot , P. A. Petitjean , L. F. Pineres Rico , A. Popov , P. Poussot , W. Pratumwan , E. Previtali , C. S. J. Pun , F. Z. Qi , M. Qi , S. Qian , X. Qian , X. H. Qian , H. Qiao , Z. H. Qin , S. K. Qiu , M. Rajput , G. Ranucci , N. Raper , A. Re , H. Rebber , A. Rebii , B. Ren , J. Ren , C. M. Reveco , T. Rezinko , B. Ricci , M. Robens , M. Roche , N. Rodphai , L. Rohwer , A. Romani , R. Rosero , B. Roskovec , C. Roth , X. C. Ruan , X. D. Ruan , S. Rujirawat , A. Rybnikov , A. Sadovsky , P. Saggese , G. Salamanna , A. Sangka , N. Sanguansak , U. Sawangwit , J. Sawatzki , F. Sawy , M. Schever , J. Schuler , C. Schwab , K. Schweizer , D. Selivanov , A. Selyunin , A. Serafini , G. Settanta , M. Settimo , M. Shahzad , G. Shi , J. Y. Shi , Y. J. Shi , V. Shutov , A. Sidorenkov , F. Simkovic , C. Sirignano , J. Siripak , M. Sisti , M. Slupecki , M. Smirnov , O. Smirnov , T. Sogo-Bezerra , J. Songwadhana , B. Soonthornthum , A. Sotnikov , O. Sramek , W. Sreethawong , A. Stahl , L. Stanco , K. Stankevich , D. Stefanik , H. Steiger , H. Steiner , J. Steinmann , M. Stender , V. Strati , A. Studenikin , G. X. Sun , L. T. Sun , J. L. Sun , S. F. Sun , X. L. Sun , Y. J. Sun , Y. Z. Sun , N. Suwonjandee , M. Szelezniak , J. Tang , Q. Tang , Q. Tang , X. Tang , A. Tietzsch , I. Tkachev , T. Tmej , K. Treskov , G. Troni , W. Trzaska , W. -H. Tse , C. E. Tull , C. Tuve , S. van Waasen , J. Vanden Boom , N. Vassilopoulos , V. Vedin , G. Verde , M. Vialkov , B. Viaud , B. Viren , C. Volpe , V. Vorobel , L. Votano , P. Walker , C. Wang , C. H. Wang , E. Wang , G. L. Wang , J. Wang , J. Wang , K. Y. Wang , L. Wang , M. F. Wang , M. Wang , M. Wang , N. Y. Wang , R. G. Wang , S. G. Wang , W. Wang , W. Wang , W. S. Wang , X. Wang , X. Y. Wang , Y. Wang , Y. Wang , Y. Wang , Y. F. Wang , Y. G. Wang , Y. M. Wang , Y. Q. Wang , Z. Wang , Z. Wang , Z. M. Wang , Z. Y. Wang , A. Watcharangkool , H. Y. Wei , L. H. Wei , W. Wei , Y. D. Wei , L. J. Wen , K. Whisnant , C. G. White , C. Wiebusch , S. C. F. Wong , H. L. H. Wong , B. Wonsak , E. Worcester , C. H. Wu , D. R. Wu , F. L. Wu , Q. Wu , W. J. Wu , Z. Wu , M. Wurm , J. Wurtz , C. Wysotzki , Y. F. Xi , D. M. Xia , Y. G. Xie , Z. Q. Xie , Z. Z. Xing , D. L. Xu , F. R. Xu , H. K. Xu , J. L. Xu , J. Xu , M. H. Xu , T. Xu , Y. Xu , Y. Xu , T. Xue , B. J. Yan , X. B. Yan , Y. P. Yan , A. B. Yang , C. G. Yang , H. Yang , J. Yang , L. Yang , X. Y. Yang , Y. F. Yang , Y. Z. Yang , H. F. Yao , Z. Yasin , J. X. Ye , M. Ye , U. Yegin , M. Yeh , F. Yermia , P. H. Yi , Z. Y. You , B. L. Young , B. X. Yu , C. X. Yu , C. Y. Yu , H. Z. Yu , M. Yu , X. H. Yu , Z. Y. Yu , C. Z. Yuan , Y. Yuan , Z. X. Yuan , Z. Y. Yuan , B. B. Yue , N. Zafar , A. Zambanini , P. Zeng , S. Zeng , T. X. Zeng , Y. D. Zeng , L. Zhan , C. Zhang , F. Y. Zhang , G. Q. Zhang , H. H. Zhang , H. Q. Zhang , J. Zhang , J. B. Zhang , J. W. Zhang , P. Zhang , Q. M. Zhang , T. Zhang , X. M. Zhang , X. T. Zhang , Y. Zhang , Y. H. Zhang , Y. M. Zhang , Y. P. Zhang , Y. X. Zhang , Y. Y. Zhang , Y. Y. Zhang , Z. J. Zhang , Z. P. Zhang , Z. Y. Zhang , Z. Y. Zhang , F. Y. Zhao , J. Zhao , R. Zhao , S. J. Zhao , T. C. Zhao , D. Q. Zheng , H. Zheng , M. S. Zheng , Y. H. Zheng , W. R. Zhong , J. Zhou , L. Zhou , N. Zhou , S. Zhou , X. Zhou , J. Zhu , K. J. Zhu , H. L. Zhuang , L. Zong , J. H. Zou

Effects of the 1-3 leptonic mixing on the solar neutrino observables are studied and the signatures of non-zero $\theta_{13}$ are identified. For this we have re-derived the formula for $3\nu$-survival probability including all relevant…

High Energy Physics - Phenomenology · Physics 2009-11-10 Srubabati Goswami , Alexei Yu. Smirnov

The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose experiment, under construction in southeast China, that is designed to determine the neutrino mass ordering and precisely measure neutrino oscillation parameters. Monte…

The determination of the neutrino mass ordering is currently pursued by several experiments and proposals. A very challenging one is its evaluation from reactor experiments based on the tiny interference effect between the $\Delta m^2_{31}$…

High Energy Physics - Phenomenology · Physics 2017-12-20 Luca Stanco , Giuseppe Salamanna , Alexey Lokhov , Fatma Sawy , Chiara Sirignano

In the context of three-neutrino oscillations, we study the possibility of using antineutrinos from nuclear reactors to explore the 10^{-4} {\rm eV^2} < \ms \ltap 8\times 10^{-4} {\rm eV^2} region of the LMA MSW solution of the solar…

High Energy Physics - Phenomenology · Physics 2009-11-07 S. T. Petcov , M. Piai

The discovery of solar neutrinos confirmed that the inner workings of the Sun generally match our theoretical understanding of the fusion process. Solar neutrinos have also played a role in discovering that neutrinos have mass and that they…

High Energy Physics - Phenomenology · Physics 2025-05-19 Peter B. Denton , Charles Gourley

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

We review the current-generation short-baseline reactor neutrino experiments that have firmly established the third neutrino mixing angle $\theta_{13}$ to be non-zero. The relative large value of $\theta_{13}$ (around 9$^\circ$) has opened…

High Energy Physics - Experiment · Physics 2014-05-29 X. Qian , W. Wang

We perform a global analysis of the latest solar neutrino data including the SNO result on the CC-event rate. This result further favors the LMA solution of the solar neutrino problem. The best fit values of parameters we find are: \Delta…

High Energy Physics - Phenomenology · Physics 2009-11-07 P. I. Krastev , A. Yu. Smirnov

We study the potential benefits of an iodine-based solar-neutrino detector for testing hypotheses that involve neutrino oscillations. We argue that such a detector will have a good chance of distinguishing the two allowed regions of $\Delta…

High Energy Physics - Phenomenology · Physics 2016-09-01 J. Engel , P. I. Krastev , K. Lande

A new underground lab, Yemilab, is being constructed in Handuk iron mine, Korea. The default design of Yemilab includes a space for a future neutrino experiment. We propose to build a water-based liquid scintillator (WbLS) detector of…

Instrumentation and Detectors · Physics 2019-03-14 Seon-Hee Seo

Results for solar neutrino detection from the SuperKamiokande collaboration have been presented recently while those from the Sudbury Neutrino Observatory are expected in the near future. These experiments are sensitive to the 8B neutrinos…

High Energy Physics - Phenomenology · Physics 2015-06-25 Debasish Majumdar , Amitava Raychaudhuri

We do a re-analysis to asses the impact of the results of the Borexino experiment and the recent 2.8 KTy KamLAND data on the solar neutrino oscillation parameters. The current Borexino results are found to have no impact on the allowed…

High Energy Physics - Phenomenology · Physics 2008-05-01 Abhijit Bandyopadhyay , Sandhya Choubey , Srubabati Goswami , S. T. Petcov , D. P. Roy

The Jiangmen Underground Neutrino Observatory (JUNO) is a large scale neutrino experiment with multiple physics goals including deter mining the neutrino mass hierarchy, the accurate measurement of neutrino oscillation parameters, the…

Instrumentation and Detectors · Physics 2024-07-08 The JUNO Collaboration

We analyze the energy spectrum of reactor neutrino events recently observed in the Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) and combine them with solar and terrestrial neutrino data, in the context of two- and…

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

We present a neutrino oscillation analysis of two particular data sets from the Daya Bay and RENO reactor neutrino experiments aiming to study the increase in precision in the oscillation parameters $\sin^2{2\theta}_{13}$ and the effective…

High Energy Physics - Phenomenology · Physics 2020-02-03 Mario A. Acero , Alexis A. Aguilar-Arevalo , Dairo J. Polo-Toledo

We explore how well reactor antineutrino experiments can constrain or measure the loss of quantum coherence in neutrino oscillations. We assume that decoherence effects are encoded in the size of the neutrino wave-packet, $\sigma$. We find…

High Energy Physics - Phenomenology · Physics 2020-08-24 André de Gouvêa , Valentina De Romeri , Christoph A. Ternes

The Jiangmen Underground Neutrino Observatory (JUNO) is a multipurpose neutrino-oscillation experiment, with a 20 kiloton liquid scintillator detector of unprecedented 3\% energy resolution (at 1 MeV) at 700-meter deep underground. There…

Instrumentation and Detectors · Physics 2019-08-13 Miao He

JUNO is a 20 kt Liquid Scintillator Antineutrino Detector currently under construction in the south of China. This report reviews JUNO's physics programme related to all neutrino sources but reactor antineutrinos, namely neutrinos from…

Instrumentation and Detectors · Physics 2016-05-31 Marco Grassi