Measurement of Neutrino and Antineutrino Oscillations Using Beam and Atmospheric Data in MINOS
P. Adamson,I. Anghel,I. Anghel,C. Backhouse,G.D. Barr,M. Bishai,Andrew Blake,G. J. Bock,D. Bogert,S. V. Cao,C. M. Castromonte,S. Childress,Joao A B Coelho,Joao A B Coelho,L. Corwin,Daniel P Cronin-Hennessy,J. K. De Jong,A. V. Devan,N. E. Devenish,M. V. Diwan,Carlos Escobar,J. J. Evans,E. Falk,G. J. Feldman,M. V. Frohne,H. R. Gallagher,R. A. Gomes,Maury Goodman,P. Gouffon,N. Graf,R. Gran,K. Grzelak,Alec Habig,S. R. Hahn,J. Hartnell,R. Hatcher,A. Himmel,A. Holin,J. Hylen,G. M. Irwin,Z. Isvan,Z. Isvan,C. James,D. A. Jensen,T. Kafka,S. M. S. Kasahara,G. Koizumi,M. Kordosky,A. E. Kreymer,Karol Lang,P. J. Litchfield,P. Lucas,W. A. Mann,Marvin L Marshak,M. Mathis,N. Mayer,A. M. McGowan,M. M. Medeiros,R. Mehdiyev,J. R. Meier,M. D. Messier,D. G. Michael,W. H. Miller,S. R. Mishra,S. Moed Sher,C. D. Moore,L. Mualem,J. A. Musser,D. Naples,J. K. Nelson,Harvey B Newman,R. J. Nichol,J. A. Nowak,J. O'Connor,W. P. Oliver,M. Orchanian,R. B. Pahlka,J. M. Paley,R. B. Patterson,Gregory J Pawloski,S. Phan-Budd,R. K. Plunkett,X. Qiu,A. Radovic,B. Rebel,C. Rosenfeld,H. A. Rubin,M. C. Sanchez,J. Schneps,A. Schreckenberger,P. Schreiner,R. Sharma,A. Sousa,N. Tagg,R. L. Talaga,Juergen Thomas,M. A. Thomson,G. Tinti,S. C. Tognini,R. Toner,D. Torretta,G. Tzanakos,J. Urheim,P. Vahle,B. Viren,A. C. Weber,R. C. Webb,Christopher G. White,L. Whitehead,L. H. Whitehead,Stanley G. Wojcicki,R. Zwaska +111 more
TLDR
Measurements of oscillation parameters from ν (μ) and ν(μ) disappearance using beam and atmospheric data from MINOS are reported, with minimal change to the neutrino parameters.Abstract:
We report measurements of oscillation parameters from ν_μ and ν_μ disappearance using beam and atmospheric data from MINOS. The data comprise exposures of 10.71×10^(20) protons on target in the ν_μ-dominated beam, 3.36×10^(20) protons on target in the ν_μ-enhanced beam, and 37.88 kton yr of atmospheric neutrinos. Assuming identical ν and ν oscillation parameters, we measure |Δm^2|=(2.41_(-0.10)^(+0.09))×10^(-3) eV^2 and sin^2(2θ)=0.950_(-0.036)^(+0.035). Allowing independent ν and ν oscillations, we measure antineutrino parameters of |Δm^2|=(2.50_(-0.25)^(+0.23))×10^(-3) eV^2 and sin^2(2θ)=0.97_(-0.08)^(+0.03), with minimal change to the neutrino parameters.read more
Citations
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Journal ArticleDOI
Global analysis of three-flavour neutrino oscillations: synergies and tensions in the determination of θ 23 , δ CP , and the mass ordering
Ivan Esteban,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,Álvaro Hernández-Cabezudo,Michele Maltoni,Thomas Schwetz +6 more
TL;DR: In this paper, a global analysis of the neutrino oscillation data available as of fall 2018 in the framework of three massive mixed neutrinos with the goal at determining the ranges of allowed values for the six relevant parameters.
Journal ArticleDOI
Neutrino Physics with JUNO
Fengpeng An,Guangpeng An,Qi An,Vito Antonelli,Eric Baussan,John F. Beacom,L. B. Bezrukov,Simon Blyth,R. Brugnera,Margherita Buizza Avanzini,Jose Busto,Anatael Cabrera,Hao Cai,Xiao Cai,Antonio Cammi,Guofu Cao,Jun Cao,Yun Chang,Shaomin Chen,S. M. Chen,Yi Chen,Davide Chiesa,Massimiliano Clemenza,Barbara Clerbaux,Janet Conrad,D. D'Angelo,Herve De Kerret,Zhi Deng,Ziyan Deng,Yayun Ding,Zelimir Djurcic,Damien Dornic,Marcos Dracos,O. Drapier,S. Dusini,Stephen T. Dye,Timo Enqvist,Donghua Fan,Jian Fang,Laurent Favart,Richard Ford,M. Göger-Neff,Haonan Gan,A. Garfagnini,Marco Giammarchi,Maxim Gonchar,Guanghua Gong,Hui Gong,M. Gonin,Marco Grassi,Christian Grewing,Mengyun Guan,Vic Guarino,Gang Guo,Wanlei Guo,Xin Heng Guo,Caren Hagner,Ran Han,Miao He,Yuekun Heng,Y. B. Hsiung,Jun Hu,Shouyang Hu,Tao Hu,Hanxiong Huang,Xingtao Huang,Lei Huo,Ara Ioannisian,Manfred Jeitler,Xiangdong Ji,Xiaoshan Jiang,Cécile Jollet,Li Kang,Michael Karagounis,Narine Kazarian,Z. V. Krumshteyn,Andre Kruth,Pasi Kuusiniemi,Tobias Lachenmaier,Rupert Leitner,Chao Li,Jiaxing Li,Wei Li,Weiguo Li,Xiaomei Li,X. N. Li,Yi Li,Yufeng Li,Zhibing Li,Hao Liang,Guey-Lin Lin,Tao Lin,Yen-Hsun Lin,Jiajie Ling,Jiajie Ling,Ivano Lippi,D. W. Liu,Hongbang Liu,Hu Liu,Jianglai Liu,Jianli Liu,Jinchang Liu,Qian Liu,Shubin Liu,Shulin Liu,Paolo Lombardi,Yongbing Long,Haoqi Lu,J. G. Lu,Jingbin Lu,Junguang Lu,Bayarto Lubsandorzhiev,Livia Ludhova,Shu Luo,Vladimir Lyashuk,R. Möllenberg,Xubo Ma,Fabio Mantovani,Yajun Mao,Stefano Maria Mari,William F. McDonough,G. Meng,Anselmo Meregaglia,E. Meroni,Mauro Mezzetto,Lino Miramonti,Thomas Mueller,Dmitry V. Naumov,Lothar Oberauer,Juan Pedro Ochoa-Ricoux,Alexander Olshevskiy,Fausto Ortica,Alessandro Paoloni,H. Peng,Jen-Chieh Peng,Ezio Previtali,Ming Qi,Sen Qian,Xin Qian,Yong Zhong Qian,Yong Zhong Qian,Zhonghua Qin,Georg G. Raffelt,Gioacchino Ranucci,Barbara Ricci,Markus Robens,Aldo Romani,Xiangdong Ruan,Xichao Ruan,G. Salamanna,M. H. Shaevitz,V. V. Sinev,Chiara Sirignano,Monica Sisti,Oleg Smirnov,M. Soiron,Achim Stahl,Luca Stanco,Jochen Steinmann,Xilei Sun,Yongjie Sun,Dmitriy Taichenachev,Jian Tang,Igor Tkachev,Wladyslaw Henryk Trzaska,Stefan van Waasen,Cristina Volpe,V. Vorobel,Lucia Votano,Chung Hsiang Wang,Guo-Li Wang,Hao Wang,Meng Wang,Ruiguang Wang,Siguang Wang,Wei Wang,Yi Wang,Yi Wang,Yifang Wang,Zhe Wang,Zheng Wang,Zheng Wang,Zhimin Wang,Wei Wei,Liangjian Wen,Christopher Wiebusch,Björn Wonsak,Qun Wu,Claudia-Elisabeth Wulz,Michael Wurm,Yufei Xi,Dongmei Xia,Yuguang Xie,Zhi-zhong Xing,Jilei Xu,Baojun Yan,Changgen Yang,C. G. Yang,Guang Yang,Lei Yang,Yifan Yang,Yu Yao,Ugur Yegin,F. Yermia,Zhengyun You,Boxiang Yu,Chunxu Yu,Zeyuan Yu,Sandra Zavatarelli,Liang Zhan,Chao Zhang,Honghao Zhang,Jiawen Zhang,Jingbo Zhang,Qingmin Zhang,Yumei Zhang,Zhenyu Zhang,Zhenghua Zhao,Yangheng Zheng,Weili Zhong,Guorong Zhou,Jing Zhou,Li Zhou,Rong Zhou,Shun Zhou,Wenxiong Zhou,Xiang Zhou,Ye-Ling Zhou,Y. H. Zhou,Jiaheng Zou +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20kton multi-purpose underground liquid scintillator detector with the determination of neutrino mass hierarchy (MH) as a primary physics goal.
Journal ArticleDOI
Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity
Ivan Esteban,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,Michele Maltoni,Ivan Martinez-Soler,Thomas Schwetz +6 more
TL;DR: In this paper, a combined fit to global neutrino oscillation data available as of fall 2016 in the scenario of three-neutrinos oscillations was performed and the allowed ranges of the six oscillation parameters were presented.
Journal ArticleDOI
The fate of hints: updated global analysis of three-flavor neutrino oscillations
Ivan Esteban,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,M. C. Gonzalez-Garcia,Michele Maltoni,Thomas Schwetz,Albert Zhou +6 more
TL;DR: In this paper, a combined analysis of the latest neutrino oscillation data presented at the Neutrino2020 conference shows that previous hints for the neutrinos mass ordering have significantly decreased, and normal ordering (NO) is favored only at the 1.6σ level.
Journal ArticleDOI
Neutrino Physics with JUNO
Fengpeng An,Guangpeng An,Qi An,Vito Antonelli,Eric Baussan,John F. Beacom,L. B. Bezrukov,Simon Blyth,R. Brugnera,Margherita Buizza Avanzini,Jose Busto,Anatael Cabrera,Hao Cai,Xiao Cai,Antonio Cammi,Guofu Cao,Jun Cao,Yun Chang,Shaomin Chen,S. M. Chen,Yi Chen,Davide Chiesa,Massimiliano Clemenza,Barbara Clerbaux,Janet Conrad,D. D'Angelo,Herve De Kerret,Zhi Deng,Ziyan Deng,Yayun Ding,Zelimir Djurcic,Damien Dornic,Marcos Dracos,O. Drapier,S. Dusini,Stephen T. Dye,Timo Enqvist,Donghua Fan,Jian Fang,Laurent Favart,Richard Ford,M. Göger-Neff,Haonan Gan,A. Garfagnini,Marco Giammarchi,Maxim Gonchar,Guanghua Gong,Hui Gong,M. Gonin,Marco Grassi,Christian Grewing,Mengyun Guan,Vic Guarino,Gang Guo,Wanlei Guo,Xin Heng Guo,Caren Hagner,Ran Han,Miao He,Yuekun Heng,Y. B. Hsiung,Jun Hu,Shouyang Hu,Tao Hu,Hanxiong Huang,Xingtao Huang,Lei Huo,Ara Ioannisian,Manfred Jeitler,Xiangdong Ji,Xiaoshan Jiang,Cécile Jollet,Li Kang,Michael Karagounis,Narine Kazarian,Z. V. Krumshteyn,Andre Kruth,Pasi Kuusiniemi,Tobias Lachenmaier,Rupert Leitner,Chao Li,Jiaxing Li,Wei Li,Weiguo Li,Xiaomei Li,X. N. Li,Yi Li,Yufeng Li,Zhibing Li,Hao Liang,Guey-Lin Lin,Tao Lin,Yen-Hsun Lin,Jiajie Ling,Jiajie Ling,Ivano Lippi,D. W. Liu,Hongbang Liu,Hu Liu,Jianglai Liu,Jianli Liu,Jinchang Liu,Qian Liu,Shubin Liu,Shulin Liu,Paolo Lombardi,Yongbing Long,Haoqi Lu,J. G. Lu,Jingbin Lu,Junguang Lu,Bayarto Lubsandorzhiev,Livia Ludhova,Shu Luo,Vladimir Lyashuk,R. Möllenberg,Xubo Ma,Fabio Mantovani,Yajun Mao,Stefano Maria Mari,William F. McDonough,G. Meng,Anselmo Meregaglia,E. Meroni,Mauro Mezzetto,Lino Miramonti,Thomas Mueller,Dmitry V. Naumov,Lothar Oberauer,Juan Pedro Ochoa-Ricoux,Alexander Olshevskiy,Fausto Ortica,Alessandro Paoloni,H. Peng,Jen-Chieh Peng,Ezio Previtali,Ming Qi,Sen Qian,Xin Qian,Yong Zhong Qian,Yong Zhong Qian,Zhonghua Qin,Georg G. Raffelt,Gioacchino Ranucci,Barbara Ricci,Markus Robens,Aldo Romani,Xiangdong Ruan,Xichao Ruan,G. Salamanna,M. H. Shaevitz,V. V. Sinev,Chiara Sirignano,Monica Sisti,Oleg Smirnov,M. Soiron,Achim Stahl,Luca Stanco,Jochen Steinmann,Xilei Sun,Yongjie Sun,Dmitriy Taichenachev,Jian Tang,Igor Tkachev,Wladyslaw Henryk Trzaska,Stefan van Waasen,Cristina Volpe,V. Vorobel,Lucia Votano,Chung Hsiang Wang,Guo-Li Wang,Hao Wang,Meng Wang,Ruiguang Wang,Siguang Wang,Wei Wang,Yi Wang,Yi Wang,Yifang Wang,Zhe Wang,Zheng Wang,Zheng Wang,Zhimin Wang,Wei Wei,Liangjian Wen,Christopher Wiebusch,Björn Wonsak,Qun Wu,Claudia-Elisabeth Wulz,Michael Wurm,Yufei Xi,Dongmei Xia,Yuguang Xie,Zhi-zhong Xing,Jilei Xu,Baojun Yan,Changgen Yang,C. G. Yang,Guang Yang,Lei Yang,Yifan Yang,Yu Yao,Ugur Yegin,F. Yermia,Zhengyun You,Boxiang Yu,Chunxu Yu,Zeyuan Yu,Sandra Zavatarelli,Liang Zhan,Chao Zhang,Honghao Zhang,Jiawen Zhang,Jingbo Zhang,Qingmin Zhang,Yumei Zhang,Zhenyu Zhang,Zhenghua Zhao,Yangheng Zheng,Weili Zhong,Guorong Zhou,Jing Zhou,Li Zhou,Rong Zhou,Shun Zhou,Wenxiong Zhou,Xiang Zhou,Ye-Ling Zhou,Y. H. Zhou,Jiaheng Zou +229 more
TL;DR: The Jiangmen Underground Neutrino Observatory (JUNO) as mentioned in this paper is a 20 kton multi-purpose underground liquid scintillator detector with the determination of the neutrino mass hierarchy as a primary physics goal.
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