JUNO is a multi-purpose neutrino observatory under construction in the south of China. This publication presents new sensitivity estimates for the measurement of the , , , and oscillation parameters using reactor antineutrinos, which is one of the primary physics goals of the experiment. The sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site, the nuclear reactors in the surrounding area and beyond, the detector response uncertainties, and the reactor antineutrino spectral shape constraints expected from the TAO satellite detector. It is found that the and oscillation parameters will be determined to 0.5% precision or better in six years of data collection. In the same period, the parameter will be determined to about % precision for each mass ordering hypothesis. The new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.
Sub-percent precision measurement of neutrino oscillation parameters with JUNO / A. Abusleme, T. Adam, S. Ahmad, R. Ahmed, S. Aiello, M. Akram, A. Aleem, F. An, Q. An, G. Andronico, N. Anfimov, V. Antonelli, T. Antoshkina, B. Asavapibhop, J. Pedro Athayde Marcondes de Andr??, D. Auguste, W. Bai, N. Balashov, W. Baldini, A. Barresi, D. Basilico, E. Baussan, M. Bellato, A. Bergnoli, T. Birkenfeld, S. Blin, D. Blum, S. Blyth, A. Bolshakova, M. Bongrand, C. Bordereau, D. Breton, A. Brigatti, R. Brugnera, R. Bruno, A. Budano, J. Busto, I. Butorov, A. Cabrera, B. Caccianiga, H. Cai, X. Cai, Y. Cai, Z. Cai, R. Callegari, A. Cammi, A. Campeny, C. Cao, G. Cao, J. Cao, R. Caruso, C. Cerna, C. Chan, J. Chang, Y. Chang, G. Chen, P. Chen, P. Chen, S. Chen, X. Chen, Y. Chen, Y. Chen, Z. Chen, Z. Chen, J. Cheng, Y. Cheng, Y. Chin Cheng, A. Chetverikov, D. Chiesa, P. Chimenti, A. Chukanov, G. Claverie, C. Clementi, B. Clerbaux, S. Conforti Di Lorenzo, D. Corti, F. Dal Corso, O. Dalager, C. De La Taille, Z. Deng, Z. Deng, W. Depnering, M. Diaz, X. Ding, Y. Ding, B. Dirgantara, S. Dmitrievsky, T. Dohnal, D. Dolzhikov, G. Donchenko, J. Dong, E. Doroshkevich, M. Dracos, F. Druillole, R. Du, S. Du, S. Dusini, M. Dvorak, T. Enqvist, H. Enzmann, A. Fabbri, D. Fan, L. Fan, J. Fang, W. Fang, M. Fargetta, D. Fedoseev, Z. Fei, L. Feng, Q. Feng, R. Ford, A. Fournier, H. Gan, F. Gao, A. Garfagnini, A. Gavrikov, M. Giammarchi, N. Giudice, M. Gonchar, G. Gong, H. Gong, Y. Gornushkin, A. G??ttel, M. Grassi, V. Gromov, M. Gu, X. Gu, Y. Gu, M. Guan, Y. Guan, N. Guardone, C. Guo, J. Guo, W. Guo, X. Guo, Y. Guo, P. Hackspacher, C. Hagner, R. Han, Y. Han, M. He, W. He, T. Heinz, P. Hellmuth, Y. Heng, R. Herrera, Y. Hor, S. Hou, Y. Hsiung, B. Hu, H. Hu, J. Hu, J. Hu, S. Hu, T. Hu, Y. Hu, Z. Hu, G. Huang, H. Huang, K. Huang, W. Huang, X. Huang, X. Huang, Y. Huang, J. Hui, L. Huo, W. Huo, C. Huss, S. Hussain, A. Ioannisian, R. Isocrate, B. Jelmini, I. Jeria, X. Ji, H. Jia, J. Jia, S. Jian, D. Jiang, W. Jiang, X. Jiang, X. Jing, C. Jollet, J. Joutsenvaara, L. Kalousis, P. Kampmann, L. Kang, R. Karaparambil, N. Kazarian, A. Khatun, K. Khosonthongkee, D. Korablev, K. Kouzakov, A. Krasnoperov, N. Kutovskiy, P. Kuusiniemi, T. Lachenmaier, C. Landini, S. Leblanc, V. Lebrin, F. Lefevre, R. Lei, R. Leitner, J. Leung, D. Li, D. Li, F. Li, F. Li, G. Li, H. Li, M. Li, M. Li, N. Li, N. Li, Q. Li, R. Li, R. Li, S. Li, T. Li, T. Li, W. Li, W. Li, X. Li, X. Li, X. Li, Y. Li, Y. Li, Y. Li, Z. Li, Z. Li, Z. Li, Z. Li, Z. Li, H. Liang, H. Liang, J. Liao, A. Limphirat, G. Lin, S. Lin, T. Lin, J. Ling, I. Lippi, F. Liu, H. Liu, H. Liu, H. Liu, H. Liu, H. Liu, H. Liu, J. Liu, J. Liu, M. Liu, Q. Liu, Q. Liu, R. Liu, S. Liu, S. Liu, X. Liu, X. Liu, Y. Liu, Y. Liu, A. Lokhov, P. Lombardi, C. Lombardo, K. Loo, C. Lu, H. Lu, J. Lu, J. Lu, S. Lu, B. Lubsandorzhiev, S. Lubsandorzhiev, L. Ludhova, A. Lukanov, D. Luo, F. Luo, G. Luo, S. Luo, W. Luo, X. Luo, V. Lyashuk, B. Ma, B. Ma, Q. Ma, S. Ma, X. Ma, X. Ma, J. Maalmi, J. Mai, Y. Malyshkin, R. Carlos Mandujano, F. Mantovani, F. Manzali, X. Mao, Y. Mao, S.M. Mari, F. Marini, C. Martellini, G. Martin-Chassard, A. Martini, M. Mayer, D. Mayilyan, I. Mednieks, A. Meinusch, Y. Meng, A. Meregaglia, E. Meroni, D. Meyh??, M. Mezzetto, J. Miller, L. Miramonti, M. Colomer Molla, P. Montini, M. Montuschi, A. M??ller, M. Nastasi, D.V. Naumov, E. Naumova, D. Navas-Nicolas, I. Nemchenok, M. Thuan Nguyen Thi, F. Ning, Z. Ning, H. Nunokawa, L. Oberauer, J. Pedro Ochoa-Ricoux, A. Olshevskiy, D. Orestano, F. Ortica, R. Othegraven, A. Paoloni, S. Parmeggiano, Y. Pei, L. Pelicci, N. Pelliccia, A. Peng, H. Peng, Y. Peng, Z. Peng, F. Perrot, P. Petitjean, F. Petrucci, O. Pilarczyk, L. Felipe Pi??eres, A. Popov, P. Poussot, E. Previtali, F. Qi, M. Qi, S. Qian, X. Qian, Z. Qian, H. Qiao, Z. Qin, S. Qiu, G. Ranucci, N. Raper, R. Rasheed, A.C. Re, H. Rebber, A. Rebii, M. Redchuk, B. Ren, J. Ren, B. Ricci, M. Rifai, M. Roche, N. Rodphai, A. Romani, B. Roskovec, X. Ruan, A. Rybnikov, A. Sadovsky, P. Saggese, S. Sanfilippo, A. Sangka, U. Sawangwit, J. Sawatzki, M. Schever, C. Schwab, K. Schweizer, A. Selyunin, A. Serafini, G. Settanta, M. Settimo, Z. Shao, V. Sharov, A. Shaydurova, J. Shi, Y. Shi, V. Shutov, A. Sidorenkov, F. ??imkovic, C. Sirignano, J. Siripak, M. Sisti, M. Slupecki, M. Smirnov, O. Smirnov, T. Sogo-Bezerra, S. Sokolov, J. Songwadhana, B. Soonthornthum, A. Sotnikov, O. ??r??mek, W. Sreethawong, A. Stahl, L. Stanco, K. Stankevich, D. ??tef??nik, H. Steiger, J. Steinmann, T. Sterr, M. Raphael Stock, V. Strati, A. Studenikin, J. Su, S. Sun, X. Sun, Y. Sun, Y. Sun, Z. Sun, N. Suwonjandee, M. Szelezniak, J. Tang, Q. Tang, Q. Tang, X. Tang, V. Thara Hariharan, E. Theisen, A. Tietzsch, I. Tkachev, T. Tmej, M. Danilo Claudio Torri, K. Treskov, A. Triossi, G. Troni, W. Trzaska, A. Tsagkarakis, C. Tuve, N. Ushakov, V. Vedin, G. Verde, M. Vialkov, B. Viaud, C. Moritz Vollbrecht, C. Volpe, K. Von Sturm, V. Vorobel, D. Voronin, L. Votano, P. Walker, C. Wang, C. Wang, E. Wang, G. Wang, J. Wang, J. Wang, L. Wang, M. Wang, M. Wang, M. Wang, R. Wang, S. Wang, W. Wang, W. Wang, W. Wang, X. Wang, X. Wang, Y. Wang, Y. Wang, Y. Wang, Y. Wang, Y. Wang, Y. Wang, Y. Wang, Z. Wang, Z. Wang, Z. Wang, Z. Wang, A. Watcharangkool, W. Wei, W. Wei, W. Wei, Y. Wei, K. Wen, L. Wen, C. Wiebusch, S. Chan-Fai Wong, B. Wonsak, D. Wu, Q. Wu, Z. Wu, M. Wurm, J. Wurtz, C. Wysotzki, Y. Xi, D. Xia, X. Xiao, X. Xie, Y. Xie, Z. Xie, Z. Xin, Z. Xing, B. Xu, C. Xu, D. Xu, F. Xu, H. Xu, J. Xu, J. Xu, M. Xu, Y. Xu, B. Yan, T. Yan, W. Yan, X. Yan, Y. Yan, C. Yang, C. Yang, H. Yang, J. Yang, L. Yang, X. Yang, Y. Yang, Y. Yang, H. Yao, J. Ye, M. Ye, Z. Ye, F. Yermia, N. Yin, Z. You, B. Yu, C. Yu, C. Yu, H. Yu, M. Yu, X. Yu, Z. Yu, Z. Yu, C. Yuan, C. Yuan, Y. Yuan, Z. Yuan, B. Yue, N. Zafar, V. Zavadskyi, S. Zeng, T. Zeng, Y. Zeng, L. Zhan, A. Zhang, B. Zhang, B. Zhang, F. Zhang, G. Zhang, H. Zhang, J. Zhang, J. Zhang, J. Zhang, J. Zhang, J. Zhang, J. Zhang, M. Zhang, P. Zhang, Q. Zhang, S. Zhang, S. Zhang, T. Zhang, X. Zhang, X. Zhang, X. Zhang, X. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Z. Zhang, Z. Zhang, F. Zhao, J. Zhao, R. Zhao, R. Zhao, S. Zhao, D. Zheng, H. Zheng, Y. Zheng, W. Zhong, J. Zhou, L. Zhou, N. Zhou, S. Zhou, T. Zhou, X. Zhou, J. Zhu, J. Zhu, K. Zhu, K. Zhu, Z. Zhu, B. Zhuang, H. Zhuang, L. Zong, J. Zou (JUNO Collaboration). - In: CHINESE PHYSICS C. - ISSN 1674-1137. - 46:12(2022), pp. 123001.123001-1-123001.123001-23. [10.1088/1674-1137/ac8bc9]
Sub-percent precision measurement of neutrino oscillation parameters with JUNO
D. Basilico;B. Caccianiga;L. Miramonti;A.C. Re;
2022
Abstract
JUNO is a multi-purpose neutrino observatory under construction in the south of China. This publication presents new sensitivity estimates for the measurement of the , , , and oscillation parameters using reactor antineutrinos, which is one of the primary physics goals of the experiment. The sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site, the nuclear reactors in the surrounding area and beyond, the detector response uncertainties, and the reactor antineutrino spectral shape constraints expected from the TAO satellite detector. It is found that the and oscillation parameters will be determined to 0.5% precision or better in six years of data collection. In the same period, the parameter will be determined to about % precision for each mass ordering hypothesis. The new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.File | Dimensione | Formato | |
---|---|---|---|
Abusleme_2022_Chinese_Phys._C_46_123001.pdf
accesso aperto
Tipologia:
Publisher's version/PDF
Dimensione
2.58 MB
Formato
Adobe PDF
|
2.58 MB | Adobe PDF | Visualizza/Apri |
Pubblicazioni consigliate
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.