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Related papers: Recent Results from KamLAND

200 papers

In this poster, we present the latest measurement of electron antineutrino disappearance using the fully constructed Daya Bay Reactor Neutrino Experiment. A total exposure of $6.9 \times 10^5$ GW$_{\mathrm{th}}$ ton days was achieved in…

High Energy Physics - Experiment · Physics 2016-05-31 Marco Grassi

We consider the impact of the recent KamLAND data on neutrino oscillations, the first terrestrial neutrino experiment that can probe the solar neutrino anomaly. By combining the first 145.1 days of KamLAND data with the full sample of…

High Energy Physics - Phenomenology · Physics 2009-09-17 M. Maltoni , T. Schwetz , J. W. F. Valle

After a logically clear and simple solution of the solar neutrino problem on the basis of the hypothesis about the existence of a new interaction involving electron neutrinos and nucleons, the question arose about the origin of the…

High Energy Physics - Phenomenology · Physics 2019-12-25 L. M. Slad

The RENO experiment reports more precisely measured values of $\theta_{13}$ and $|\Delta m_{ee}^2|$ using $\sim$2\,200 live days of data. The amplitude and frequency of reactor electron antineutrino ($\overline{\nu}_e$) oscillation are…

KamLAND is a reactor neutrino oscillation experiment with a very long baseline. This experiment successfully measured oscillation phenomena of reactor antineutrinos coming mainly from 53 reactors in Japan. In order to extract the results,…

Data Analysis, Statistics and Probability · Physics 2008-11-26 K. Nakajima , K. Inoue , K. Owada , F. Suekane , A. Suzuki , G. Hirano , S. Kosaka , T. Ohta , H. Tanaka

The Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) is sensitive to the neutrino event spectrum from (mainly Japanese) nuclear reactors in both the energy domain and the time domain. While the energy spectrum of KamLAND events…

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

KamLAND is a massive liquid-scintillator-based neutrino detector studying low energy neutrino oscillation. The experiment has discovered a large deficit of the reactor neutrino flux with baseline of 180km in the year 2002. This result is…

Instrumentation and Detectors · Physics 2019-08-14 F. Suekane , T. Iwamoto , H. Ogawa , O. Tajima , H. Watanabe

The Reactor Experiment for Neutrino Oscillation (RENO) experiment has been taking data using two identical liquid scintillator detectors of 44.5 tons since August 2011. The experiment has observed the disappearance of reactor neutrinos in…

Possible mixing of the active and sterile neutrinos has been considered both in the single Delta m^2 approximation and in the case of more than one Delta m^2. We perform global fit of the available solar neutrino data with free boron…

High Energy Physics - Phenomenology · Physics 2007-05-23 P. C. de Holanda , A. Yu. Smirnov

The Reactor Experiment for Neutrino Oscillation (RENO) has been taking electron antineutrino ($\overline{\nu}_{e}$) data from the reactors in Yonggwang, Korea, using two identical detectors since August 2011. Using roughly 500 live days of…

The Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) is used in a search for single neutron or two neutron intra-nuclear disappearance that would produce holes in the $\it{s}$-shell energy level of $^{12}$C nuclei. Such holes…

High Energy Physics - Experiment · Physics 2012-08-27 The KamLAND collaboration

A maximum likelihood approach has been used to analize the first results from KamLAND emphasizing the application of this method for low statistics samples. The goodness of fit has been determined exploiting a simple Monte Carlo approach in…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. Ianni

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

We report a search result for a light sterile neutrino oscillation with roughly 2200 live days of data in the RENO experiment. The search is performed by electron antineutrino ($\overline{\nu}_e$) disappearance taking place between six 2.8…

The SNO+ collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 tonne-years of new data. The measured energies of reactor antineutrino candidates were fitted to obtain the second-most precise…

High Energy Physics - Experiment · Physics 2025-09-18 SNO+ Collaboration , : , M. Abreu , V. Albanese , A. Allega , R. Alves , M. R. Anderson , S. Andringa , L. Anselmo , J. Antunes , E. Arushanova , S. Asahi , M. Askins , D. M. Asner , D. J. Auty , A. R. Back , S. Back , A. Bacon , T. Baltazar , F. Barão , Z. Barnard , A. Barr , N. Barros , D. Bartlett , R. Bayes , C. Beaudoin , E. W. Beier , G. Berardi , T. S. Bezerra , A. Bialek , S. D. Biller , E. Blucher , A. Boeltzig , R. Bonventre , M. Boulay , D. Braid , E. Caden , E. J. Callaghan , J. Caravaca , J. Carvalho , L. Cavalli , D. Chauhan , M. Chen , S. Cheng , O. Chkvorets , K. J. Clark , B. Cleveland , C. Connors , D. Cookman , J. Corning , I. T. Coulter , M. A. Cox , D. Cressy , X. Dai , C. Darrach , S. DeGraw , R. Dehghani , J. Deloye , M. M. Depatie , F. Descamps , C. Dima , J. Dittmer , K. H. Dixon , F. Di Lodovico , A. Doxtator , N. Duhaime , F. Duncan , J. Dunger , A. D. Earle , M. S. Esmaeilian , D. Fabris , E. Falk , A. Farrugia , N. Fatemighomi , C. Felber , V. Fischer , E. Fletcher , R. Ford , K. Frankiewicz , N. Gagnon , A. Gaur , J. Gauthier , A. Gibson-Foster , K. Gilje , O. I. González-Reina , D. Gooding , P. Gorel , K. Graham , C. Grant , J. Grove , S. Grullon , E. Guillian , R. L. Hahn , S. Hall , A. L. Hallin , D. Hallman , S. Hans , J. Hartnell , P. Harvey , C. Hearns , M. R. Hebert , M. Hedayatipour , W. J. Heintzelman , J. Heise , R. L. Helmer , C. Hewitt , B. Hodak , M. Hodak , M. Hood , D. Horne , M. Howe , B. Hreljac , J. Hu , P. Huang , R. Hunt-Stokes , T. Iida , A. S. Inácio , C. M. Jackson , N. A. Jelley , C. J. Jillings , C. Jones , P. G. Jones , S. Kaluzienski , K. Kamdin , T. Kaptanoglu , J. Kaspar , K. Keeter , C. Kefelian , P. Khaghani , L. Kippenbrock , J. Kladnik , J. R. Klein , R. Knapik , J. Kofron , L. L. Kormos , S. Korte , B. Krar , C. Kraus , C. B. Krauss , T. Kroupová , K. Labe , F. Lafleur , C. Lake , I. Lam , C. Lan , B. J. Land , R. Lane , S. Langrock , P. Larochelle , S. Larose , A. LaTorre , I. Lawson , L. Lebanowski , J. Lee , C. Lefebvre , G. M. Lefeuvre , E. J. Leming , A. Li , O. Li , J. Lidgard , B. Liggins , P. Liimatainen , Y. H. Lin , X. Liu , Y. Liu , V. Lozza , M. Luo , S. Maguire , A. Maio , K. Majumdar , S. Manecki , J. Maneira , R. D. Martin , E. Marzec , A. Mastbaum , A. Mathewson , N. McCauley , A. B. McDonald , K. McFarlane , P. Mekarski , M. Meyer , C. Miller , C. Mills , G. Milton , M. Mlejnek , E. Mony , B. Morissette , D. Morris , I. Morton-Blake , M. J. Mottram , M. Mubasher , S. Nae , S. Naugle , M. Newcomer , M. Nirkko , L. J. Nolan , V. M. Novikov , H. M. O'Keeffe , E. O'Sullivan , G. D. Orebi Gann , S. Ouyang , J. Page , S. Pal , K. Paleshi , W. Parker , M. J. Parnell , J. Paton , S. J. M. Peeters , T. Pershing , Z. Petriw , J. Petzoldt , L. J. Pickard , D. Pracsovics , G. Prior , J. C. Prouty , B. Quenallata , S. Quirk , P. Ravi , S. Read , A. Reichold , M. Reinhard , S. Riccetto , M. Rigan , I. Ritchie , A. Robertson , B. C. Robertson , J. Rose , R. Rosero , P. M. Rost , J. Rumleskie , A. Sörensen , P. Schrock , M. A. Schumaker , M. H. Schwendener , D. Scislowski , J. Secrest , M. Seddighin , L. Segui , S. Seibert , I. Semenec , F. Shaker , T. Shantz , M. K. Sharma , J. Shen , T. M. Shokair , L. Sibley , J. Simms , J. R. Sinclair , K. Singh , P. Skensved , M. Smiley , T. Sonley , M. St-Amant , R. Stainforth , S. Stankiewicz , M. Strait , M. I. Stringer , A. Stripay , R. Svoboda , S. Tacchino , R. Tafirout , B. Tam , C. Tanguay , J. Tatar , L. Tian , N. Tolich , J. Tseng , H. W. C. Tseung , E. Turner , E. Vázquez-Jáuregui , S. Valder , R. Van Berg , J. G. C. Veinot , C. J. Virtue , B. von Krosigk , J. M. G. Walker , M. Walker , J. Wallig , S. C. Walton , F. Wang , J. Wang , M. Ward , J. Waterfield , J. J. Weigand , R. F. White , J. F. Wilkerson , J. R. Wilson , J. D. Wilson , T. J. Winchester , P. Woosaree , A. Wright , S. Yang , K. Yazigi , Z. Ye , M. Yeh , S. Yu , T. Zhang , Y. Zhang , T. Zhao , K. Zuber , A. Zummo

We present an updated analysis of all available solar and reactor neutrino data, emphasizing in particular the totality of the KamLAND (314d live time) results and including for the first time the solar $SNO$ (391d live time, phase II…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Antonelli , E. Torrente-Lujan

We present new constraints on the neutrino oscillation parameters $/textyen Delta m^{2}_{21}$, $/textyen theta_{12}$, and $/textyen theta_{13}$ from a three-flavor analysis of solar and KamLAND data. The KamLAND data set includes data…

High Energy Physics - Experiment · Physics 2012-08-27 The KamLAND Collaboration

We report a new measurement of electron antineutrino disappearance using the fully-constructed Daya Bay Reactor Neutrino Experiment. The final two of eight antineutrino detectors were installed in the summer of 2012. Including the 404 days…

High Energy Physics - Experiment · Physics 2015-09-16 Daya Bay Collaboration , F. P. An , A. B. Balantekin , H. R. Band , M. Bishai , S. Blyth , I. Butorov , G. F. Cao , J. Cao , W. R. Cen , Y. L. Chan , J. F. Chang , L. C. Chang , Y. Chang , H. S. Chen , Q. Y. Chen , S. M. Chen , Y. X. Chen , Y. Chen , J. H. Cheng , J. Cheng , Y. P. Cheng , J. J. Cherwinka , M. C. Chu , J. P. Cummings , J. de Arcos , Z. Y. Deng , X. F. Ding , Y. Y. Ding , M. V. Diwan , E. Draeger , D. A. Dwyer , W. R. Edwards , S. R. Ely , R. Gill , M. Gonchar , G. H. Gong , H. Gong , M. Grassi , W. Q. Gu , M. Y. Guan , L. Guo , X. H. Guo , R. W. Hackenburg , R. Han , S. Hans , M. He , K. M. Heeger , Y. K. Heng , Y. K. Hor , Y. B. Hsiung , B. Z. Hu , L. M. Hu , L. J. Hu , T. Hu , W. Hu , E. C. Huang , H. X. Huang , X. T. Huang , P. Huber , G. Hussain , D. E. Jaffe , P. Jaffke , K. L. Jen , S. Jetter , X. P. Ji , X. L. Ji , J. B. Jiao , R. A. Johnson , L. Kang , S. H. Kettell , M. Kramer , K. K. Kwan , M. W. Kwok , T. Kwok , T. J. Langford , K. Lau , L. Lebanowski , J. Lee , R. T. Lei , R. Leitner , A. Leung , J. K. C. Leung , C. A. Lewis , D. J. Li , F. Li , G. S. Li , Q. J. Li , S. C. Li , W. D. Li , X. N. Li , X. Q. Li , Y. F. Li , Z. B. Li , H. Liang , C. J. Lin , G. L. Lin , P. Y. Lin , S. K. Lin , J. J. Ling , J. M. Link , L. Littenberg , B. R. Littlejohn , D. W. Liu , H. Liu , J. L. Liu , J. C. Liu , S. S. Liu , C. Lu , H. Q. Lu , J. S. Lu , K. B. Luk , Q. M. Ma , X. Y. Ma , X. B. Ma , Y. Q. Ma , K. T. McDonald , R. D. McKeown , Y. Meng , I. Mitchell , J. Monari Kebwaro , Y. Nakajima , J. Napolitano , D. Naumov , E. Naumova , H. Y. Ngai , Z. Ning , J. P. Ochoa-Ricoux , A. Olshevski , S. Patton , V. Pec , J. C. Peng , L. E. Piilonen , L. Pinsky , C. S. J. Pun , F. Z. Qi , M. Qi , X. Qian , N. Raper , B. Ren , J. Ren , R. Rosero , B. Roskovec , X. C. Ruan , B. B. Shao , H. Steiner , G. X. Sun , J. L. Sun , W. Tang , H. Themann , K. V. Tsang , C. E. Tull , Y. C. Tung , N. Viaux , B. Viren , V. Vorobel , C. H. Wang , M. Wang , N. Y. Wang , R. G. Wang , W. Wang , W. W. Wang , X. Wang , Y. F. Wang , Z. Wang , Z. Wang , Z. M. Wang , H. Y. Wei , L. J. Wen , K. Whisnant , C. G. White , L. Whitehead , T. Wise , H. L. H. Wong , S. C. F. Wong , E. Worcester , Q. Wu , D. M. Xia , J. K. Xia , X. Xia , Z. Z. Xing , J. Y. Xu , J. L. Xu , J. Xu , Y. Xu , T. Xue , J. Yan , C. G. Yang , L. Yang , M. S. Yang , M. T. Yang , M. Ye , M. Yeh , Y. S. Yeh , B. L. Young , G. Y. Yu , Z. Y. Yu , S. L. Zang , L. Zhan , C. Zhang , H. H. Zhang , J. W. Zhang , Q. M. Zhang , Y. M. Zhang , Y. X. Zhang , Y. M. Zhang , Z. J. Zhang , Z. Y. Zhang , Z. P. Zhang , J. Zhao , Q. W. Zhao , Y. F. Zhao , Y. B. Zhao , L. Zheng , W. L. Zhong , L. Zhou , N. Zhou , H. L. Zhuang , J. H. Zou

We use the recently reported KamLAND measurements on oscillations of reactor anti-neutrinos, together with the data of previously reported solar neutrino experiments, to show that: (1) the total 8B neutrino flux emitted by the Sun is…

High Energy Physics - Phenomenology · Physics 2010-02-03 John N. Bahcall , M. C. Gonzalez-Garcia , Carlos Pena-Garay