JUNO sensitivity to 7Be, pep, and CNO solar neutrinos

Abusleme, A.; Adam, T.; Ahmad, S.; Ahmed, R.; Aiello, S.; Akram, M.; Aleem, A.; Alexandros, T.; Fengpeng, A.; Qi, A.; Andronico, G.; Anfimov, N.; Antonelli, V.; Antoshkina, T.; Asavapibhop, B.; de André, J.P.A.M.; Auguste, D.; Bai, W.; Balashov, N.; Baldini, W.; Barresi, A.; Basilico, D.; Baussan, E.; Bellato, M.; Beretta, M.; Bergnoli, A.; Bick, D.; Bieger, L.; Biktemerova, S.; Birkenfeld, T.; Blum, D.; Blyth, S.; Bolshakova, A.; Bongrand, M.; Bordereau, C.; Breton, D.; Brigatti, A.; Brugnera, R.; Bruno, R.; Budano, A.; Busto, J.; Cabrera, A.; Caccianiga, B.; Cai, H.; Cai, X.; Cai, Y.; Cai, Z.; Callier, S.; Cammi, A.; Campeny, A.; Cao, C.; Cao, G.; Cao, J.; Caruso, R.; Cerna, C.; Cerrone, V.; Chan, C.; Chang, J.; Chang, Y.; Chen, C.; Chen, G.; Chen, P.; Chen, S.; Chen, Y.; Chen, Y.; Chen, Z.; Chen, Z.; Cheng, J.; Cheng, Y.; Cheng, Y.C.; Chepurnov, A.; Chetverikov, A.; Chiesa, D.; Chimenti, P.; Chu, Z.; Chukanov, A.; Claverie, G.; Clementi, C.; Clerbaux, B.; Molla, M.C.; Lorenzo, S.C.D.; Coppi, A.; Corti, D.; Csakli, S.; Corso, F.D.; Dalager, O.; Datta, J.; Taille, C.D.L.; Deng, Z.; Deng, Z.; Depnering, W.; Ding, X.; Ding, X.; Ding, Y.; Dirgantara, B.; Dittrich, C.; Dmitrievsky, S.; Dohnal, T.; Dolzhikov, D.; Donchenko, G.; Dong, J.; Doroshkevich, E.; Dou, W.; Dracos, M.; Druillole, F.; Ran, D.; Shuxian, D.; Dugas, K.; Dusini, S.; Duyang, H.; Eck, J.; Enqvist, T.; Fabbri, A.; Fahrendholz, U.; Fan, L.; Fang, J.; Fang, W.; Fargetta, M.; Fedoseev, D.; Fei, Z.; Feng, L.; Feng, Q.; Ferraro, F.; Fournier, A.; Gan, H.; Gao, F.; Garfagnini, A.; Gavrikov, A.; Giammarchi, M.; Giudice, N.; Gonchar, M.; Gong, G.; Gong, H.; Gornushkin, Y.; Göttel, A.; Grassi, M.; Gromov, M.; Gromov, V.; Minghao, G.; Xiaofei, G.; Yu, G.; Guan, M.; Guan, Y.; Guardone, N.; Guo, C.; Guo, W.; Guo, X.; Hagner, C.; Han, R.; Han, Y.; Miao, H.; Wei, H.; Heinz, T.; Hellmuth, P.; Heng, Y.; Herrera, R.; Hor, Y.; Hou, S.; Hsiung, Y.; Bei-Zhen, H.; Hang, H.; Jianrun, H.; Jun, H.; Shouyang, H.; Tao, H.; Yuxiang, H.; Zhuojun, H.; Huang, G.; Huang, H.; Huang, J.; Huang, J.; Huang, K.; Huang, W.; Huang, X.; Huang, X.; Huang, Y.; Hui, J.; Huo, L.; Huo, W.; Huss, C.; Hussain, S.; Imbert, L.; Ioannisian, A.; Isocrate, R.; Jelmini, B.; Jeria, I.; Xiaolu, J.; Jia, H.; Jia, J.; Jian, S.; Jiang, C.; Jiang, D.; Jiang, W.; Jiang, X.; Jing, X.; Jollet, C.; Kampmann, P.; Kang, L.; Karaparambil, R.; Kazarian, N.; Khan, A.; Khatun, A.; Khosonthongkee, K.; Korablev, D.; Kouzakov, K.; Krasnoperov, A.; Kuleshov, S.; Kutovskiy, N.; Lachenmaier, T.; Landini, C.; Leblanc, S.; Lebrin, V.; Lefevre, F.; Lei, R.; Leitner, R.; Leung, J.; Demin, L.; Fei, L.; Fule, L.; Gaosong, L.; Huiling, L.; Jiajun, L.; Mengzhao, L.; Min, L.; Nan, L.; Qingjiang, L.; Ruhui, L.; Rui, L.; Shanfeng, L.; Tao, L.; Teng, L.; Weidong, L.; Weiguo, L.; Xiaomei, L.; Xiaonan, L.; Xinglong, L.; Yi, L.; Yichen, L.; Yufeng, L.; Zepeng, L.; Zhaohan, L.; Zhibing, L.; Ziyuan, L.; Zonghai, L.; Liang, H.; Liang, H.; Liao, J.; Limphirat, A.; Lin, G.; Lin, S.; Lin, T.; Ling, J.; Ling, X.; Lippi, I.; Liu, C.; Liu, F.; Liu, F.; Liu, H.; Liu, H.; Liu, H.; Liu, H.; Liu, H.; Liu, H.; Liu, J.; Liu, J.; Liu, J.; Liu, M.; Liu, Q.; Liu, Q.; Liu, R.; Liu, S.; Liu, S.; Liu, S.; Liu, X.; Liu, X.; Liu, X.; Liu, Y.; Liu, Z.; Lokhov, A.; Lombardi, P.; Lombardo, C.; Loo, K.; Chuan, L.; Haoqi, L.; Jingbin, L.; Junguang, L.; Peizhi, L.; Shuxiang, L.; Lubsandorzhiev, B.; Lubsandorzhiev, S.; Ludhova, L.; Lukanov, A.; Luo, D.; Luo, F.; Luo, G.; Luo, J.; Luo, S.; Luo, W.; Luo, X.; Lyashuk, V.; Bangzheng, M.; Bing, M.; Qiumei, M.; Si, M.; Xiaoyan, M.; Xubo, M.; Maalmi, J.; Magoni, M.; Mai, J.; Malyshkin, Y.; Mandujano, R.C.; Mantovani, F.; Mao, X.; Mao, Y.; Mari, S.M.; Marini, F.; Martini, A.; Mayer, M.; Mayilyan, D.; Mednieks, I.; Meng, Y.; Meraviglia, A.; Meregaglia, A.; Meroni, E.; Meyhöfer, D.; Miramonti, L.; Mohan, N.; Montini, P.; Montuschi, M.; Müller, A.; Nastasi, M.; Naumov, D.V.; Naumova, E.; Navas-Nicolas, D.; Nemchenok, I.; Thi, M.T.N.; Nikolaev, A.; Ning, F.; Ning, Z.; Nunokawa, H.; Oberauer, L.; Ochoa-Ricoux, J.P.; Olshevskiy, A.; Orestano, D.; Ortica, F.; Othegraven, R.; Paoloni, A.; Parmeggiano, S.; Pei, Y.; Pelicci, L.; Peng, A.; Peng, H.; Peng, Y.; Peng, Z.; Perrot, F.; Petitjean, P.; Petrucci, F.; Pilarczyk, O.; Rico, L.F.P.; Popov, A.; Poussot, P.; Previtali, E.; Fazhi, Q.; Ming, Q.; Xiaohui, Q.; Qian, S.; Qian, X.; Qian, Z.; Qiao, H.; Qin, Z.; Qiu, S.; Ranucci, G.; Rasheed, R.; Re, A.C.; Rebii, A.; Redchuk, M.; Ren, B.; Ren, J.; Ricci, B.; Rifai, M.; Roche, M.; Rodphai, N.; Romani, A.; Roskovec, B.; Ruan, X.; Rybnikov, A.; Sadovsky, A.; Saggese, P.; Sandanayake, D.; Sanfilippo, S.; Sangka, A.; Sawangwit, U.; Schever, M.; Schwab, C.; Schweizer, K.; Selyunin, A.; Serafini, A.; Settimo, M.; Sharov, V.; Shaydurova, A.; Shi, J.; Shi, Y.; Shutov, V.; Sidorenkov, A.; Šimkovic, F.; Singhal, A.; Sirignano, C.; Siripak, J.; Sisti, M.; Smirnov, M.; Smirnov, O.; Sogo-Bezerra, T.; Sokolov, S.; Songwadhana, J.; Soonthornthum, B.; Sotnikov, A.; Šrámek, O.; Sreethawong, W.; Stahl, A.; Stanco, L.; Stankevich, K.; Steiger, H.; Steinmann, J.; Sterr, T.; Stock, M.R.; Strati, V.; Studenikin, A.; Jun, S.; Sun, S.; Sun, X.; Sun, Y.; Sun, Y.; Sun, Z.; Suwonjandee, N.; Szelezniak, M.; Takenaka, A.; Tang, J.; Tang, Q.; Tang, Q.; Tang, X.; Hariharan, V.T.; Theisen, E.; Tietzsch, A.; Tkachev, I.; Tmej, T.; Torri, M.D.C.; Tortorici, F.; Treskov, K.; Triossi, A.; Triozzi, R.; Trzaska, W.; Tung, Y.; Tuve, C.; Ushakov, N.; Vedin, V.; Verde, G.; Vialkov, M.; Viaud, B.; Vollbrecht, C.M.; von Sturm, K.; Vorobel, V.; Voronin, D.; Votano, L.; Walker, P.; Wang, C.; Wang, C.; Wang, E.; Wang, G.; Wang, J.; Wang, J.; Wang, L.; Wang, M.; Wang, M.; Wang, R.; Wang, S.; 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.; Watcharangkool, A.; Wei, W.; Wei, W.; Wei, W.; Wei, Y.; Wen, K.; Wen, L.; Weng, J.; Wiebusch, C.; Wirth, R.; Wonsak, B.; Diru, W.; Qun, W.; Yiyang, W.; Zhi, W.; Wurm, M.; Wurtz, J.; Wysotzki, C.; Yufei, X.; Xia, D.; Xiao, X.; Xie, X.; Xie, Y.; Xie, Z.; Xin, Z.; Xing, Z.; Benda, X.; Cheng, X.; Donglian, X.; Fanrong, X.; Hangkun, X.; Jilei, X.; Jing, X.; Meihang, X.; Yin, X.; Yu, X.; Yan, B.; Yan, Q.; Yan, T.; Yan, X.; Yan, Y.; Yang, C.; Yang, C.; Yang, J.; Yang, L.; Yang, X.; Yang, Y.; Yang, Y.; Yao, H.; Jiaxuan, Y.; Mei, Y.; Ziping, Y.; Yermia, F.; You, Z.; Boxiang, Y.; Chiye, Y.; Chunxu, Y.; Guojun, Y.; Hongzhao, Y.; Miao, Y.; Xianghui, Y.; Zeyuan, Y.; Zezhong, Y.; Yuan, C.; Yuan, C.; Yuan, Y.; Yuan, Z.; Yue, B.; Zafar, N.; Zavadskyi, V.; Zeng, S.; Zeng, T.; Zeng, Y.; Zhan, L.; Zhang, A.; Zhang, B.; Zhang, B.; Zhang, F.; Zhang, H.; Zhang, H.; Zhang, J.; Zhang, J.; Zhang, J.; Zhang, J.; Zhang, J.; Zhang, M.; Zhang, P.; Zhang, Q.; Zhang, S.; Zhang, S.; Zhang, S.; Zhang, S.; Zhang, T.; Zhang, X.; Zhang, X.; Zhang, X.; Zhang, Y.; Zhang, Y.; Zhang, Y.; Zhang, Y.; Zhang, Y.; Zhang, Y.; Zhang, Z.; Zhang, Z.; Zhao, J.; Zhao, R.; Zhao, R.; Zhao, S.; Zheng, D.; Zheng, H.; Zheng, Y.; Zhong, W.; Zhou, J.; Zhou, L.; Zhou, N.; Zhou, S.; Zhou, T.; Zhou, X.; Zhu, J.; Zhu, K.; Zhu, K.; Zhu, Z.; Zhuang, B.; Zhuang, H.; Zong, L.; Zou, J.; Züfle, J.; Zwickel, S.

doi:10.1088/1475-7516/2023/10/022

The Jiangmen Underground Neutrino Observatory (JUNO), the first multi-kton liquid scintillator detector, which is under construction in China, will have a unique potential to perform a real-time measurement of solar neutrinos well below the few MeV threshold typical of Water Cherenkov detectors. JUNO's large target mass and excellent energy resolution are prerequisites for reaching unprecedented levels of precision. In this paper, we provide estimation of the JUNO sensitivity to 7Be, pep, and CNO solar neutrinos that can be obtained via a spectral analysis above the 0.45 MeV threshold. This study is performed assuming different scenarios of the liquid scintillator radiopurity, ranging from the most optimistic one corresponding to the radiopurity levels obtained by the Borexino experiment, up to the minimum requirements needed to perform the neutrino mass ordering determination with reactor antineutrinos — the main goal of JUNO. Our study shows that in most scenarios, JUNO will be able to improve the current best measurements on 7Be, pep, and CNO solar neutrino fluxes. We also perform a study on the JUNO capability to detect periodical time variations in the solar neutrino flux, such as the day-night modulation induced by neutrino flavor regeneration in Earth, and the modulations induced by temperature changes driven by helioseismic waves.

JUNO sensitivity to 7Be, pep, and CNO solar neutrinos / A. Abusleme, T. Adam, S. Ahmad, R. Ahmed, S. Aiello, M. Akram, A. Aleem, T. Alexandros, F. An, Q. An, G. Andronico, N. Anfimov, V. Antonelli, T. Antoshkina, B. Asavapibhop, J.P.A.M. de André, D. Auguste, W. Bai, N. Balashov, W. Baldini, A. Barresi, D. Basilico, E. Baussan, M. Bellato, M. Beretta, A. Bergnoli, D. Bick, L. Bieger, S. Biktemerova, T. Birkenfeld, D. Blum, S. Blyth, A. Bolshakova, M. Bongrand, C. Bordereau, D. Breton, A. Brigatti, R. Brugnera, R. Bruno, A. Budano, J. Busto, A. Cabrera, B. Caccianiga, H. Cai, X. Cai, Y. Cai, Z. Cai, S. Callier, A. Cammi, A. Campeny, C. Cao, G. Cao, J. Cao, R. Caruso, C. Cerna, V. Cerrone, C. Chan, J. Chang, Y. Chang, C. Chen, G. Chen, P. Chen, S. Chen, Y. Chen, Y. Chen, Z. Chen, Z. Chen, J. Cheng, Y. Cheng, Y.C. Cheng, A. Chepurnov, A. Chetverikov, D. Chiesa, P. Chimenti, Z. Chu, A. Chukanov, G. Claverie, C. Clementi, B. Clerbaux, M.C. Molla, S.C.D. Lorenzo, A. Coppi, D. Corti, S. Csakli, F.D. Corso, O. Dalager, J. Datta, C.D.L. Taille, Z. Deng, Z. Deng, W. Depnering, X. Ding, X. Ding, Y. Ding, B. Dirgantara, C. Dittrich, S. Dmitrievsky, T. Dohnal, D. Dolzhikov, G. Donchenko, J. Dong, E. Doroshkevich, W. Dou, M. Dracos, F. Druillole, R. Du, S. Du, K. Dugas, S. Dusini, H. Duyang, J. Eck, T. Enqvist, A. Fabbri, U. Fahrendholz, L. Fan, J. Fang, W. Fang, M. Fargetta, D. Fedoseev, Z. Fei, L. Feng, Q. Feng, F. Ferraro, A. Fournier, H. Gan, F. Gao, A. Garfagnini, A. Gavrikov, M. Giammarchi, N. Giudice, M. Gonchar, G. Gong, H. Gong, Y. Gornushkin, A. Göttel, M. Grassi, M. Gromov, V. Gromov, M. Gu, X. Gu, Y. Gu, M. Guan, Y. Guan, N. Guardone, C. Guo, W. Guo, X. Guo, 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, J. Huang, J. Huang, K. Huang, W. Huang, X. Huang, X. Huang, Y. Huang, J. Hui, L. Huo, W. Huo, C. Huss, S. Hussain, L. Imbert, A. Ioannisian, R. Isocrate, B. Jelmini, I. Jeria, X. Ji, H. Jia, J. Jia, S. Jian, C. Jiang, D. Jiang, W. Jiang, X. Jiang, X. Jing, C. Jollet, P. Kampmann, L. Kang, R. Karaparambil, N. Kazarian, A. Khan, A. Khatun, K. Khosonthongkee, D. Korablev, K. Kouzakov, A. Krasnoperov, S. Kuleshov, N. Kutovskiy, T. Lachenmaier, C. Landini, S. Leblanc, V. Lebrin, F. Lefevre, R. Lei, R. Leitner, J. Leung, D. Li, F. Li, F. Li, G. Li, H. Li, J. Li, M. Li, M. 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, X. Ling, I. Lippi, C. Liu, F. Liu, F. Liu, H. Liu, H. Liu, H. Liu, H. Liu, H. Liu, H. Liu, J. Liu, J. Liu, J. Liu, M. Liu, Q. Liu, Q. Liu, R. Liu, S. Liu, S. Liu, S. Liu, X. Liu, X. Liu, X. Liu, Y. Liu, Z. Liu, A. Lokhov, P. Lombardi, C. Lombardo, K. Loo, C. Lu, H. Lu, J. Lu, J. Lu, P. Lu, S. Lu, B. Lubsandorzhiev, S. Lubsandorzhiev, L. Ludhova, A. Lukanov, D. Luo, F. Luo, G. Luo, J. Luo, S. Luo, W. Luo, X. Luo, V. Lyashuk, B. Ma, B. Ma, Q. Ma, S. Ma, X. Ma, X. Ma, J. Maalmi, M. Magoni, J. Mai, Y. Malyshkin, R.C. Mandujano, F. Mantovani, X. Mao, Y. Mao, S.M. Mari, F. Marini, A. Martini, M. Mayer, D. Mayilyan, I. Mednieks, Y. Meng, A. Meraviglia, A. Meregaglia, E. Meroni, D. Meyhöfer, L. Miramonti, N. Mohan, P. Montini, M. Montuschi, A. Müller, M. Nastasi, D.V. Naumov, E. Naumova, D. Navas-Nicolas, I. Nemchenok, M.T.N. Thi, A. Nikolaev, F. Ning, Z. Ning, H. Nunokawa, L. Oberauer, J.P. Ochoa-Ricoux, A. Olshevskiy, D. Orestano, F. Ortica, R. Othegraven, A. Paoloni, S. Parmeggiano, Y. Pei, L. Pelicci, A. Peng, H. Peng, Y. Peng, Z. Peng, F. Perrot, P. Petitjean, F. Petrucci, O. Pilarczyk, L.F.P. Rico, A. Popov, P. Poussot, E. Previtali, F. Qi, M. Qi, X. Qi, S. Qian, X. Qian, Z. Qian, H. Qiao, Z. Qin, S. Qiu, G. Ranucci, R. Rasheed, A.C. Re, 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, D. Sandanayake, S. Sanfilippo, A. Sangka, U. Sawangwit, M. Schever, C. Schwab, K. Schweizer, A. Selyunin, A. Serafini, M. Settimo, V. Sharov, A. Shaydurova, J. Shi, Y. Shi, V. Shutov, A. Sidorenkov, F. Šimkovic, A. Singhal, C. Sirignano, J. Siripak, M. Sisti, M. Smirnov, O. Smirnov, T. Sogo-Bezerra, S. Sokolov, J. Songwadhana, B. Soonthornthum, A. Sotnikov, O. Šrámek, W. Sreethawong, A. Stahl, L. Stanco, K. Stankevich, H. Steiger, J. Steinmann, T. Sterr, M.R. Stock, V. Strati, A. Studenikin, J. Su, S. Sun, X. Sun, Y. Sun, Y. Sun, Z. Sun, N. Suwonjandee, M. Szelezniak, A. Takenaka, J. Tang, Q. Tang, Q. Tang, X. Tang, V.T. Hariharan, E. Theisen, A. Tietzsch, I. Tkachev, T. Tmej, M.D.C. Torri, F. Tortorici, K. Treskov, A. Triossi, R. Triozzi, W. Trzaska, Y. Tung, C. Tuve, N. Ushakov, V. Vedin, G. Verde, M. Vialkov, B. Viaud, C.M. Vollbrecht, 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, R. Wang, S. 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, A. Watcharangkool, W. Wei, W. Wei, W. Wei, Y. Wei, K. Wen, L. Wen, J. Weng, C. Wiebusch, R. Wirth, B. Wonsak, D. Wu, Q. Wu, Y. 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, Y. Xu, B. Yan, Q. Yan, T. Yan, X. Yan, Y. Yan, C. Yang, C. Yang, J. Yang, L. Yang, X. Yang, Y. Yang, Y. Yang, H. Yao, J. Ye, M. Ye, Z. Ye, F. Yermia, Z. You, B. Yu, C. Yu, C. Yu, G. 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, H. Zhang, H. Zhang, J. Zhang, J. Zhang, J. Zhang, J. Zhang, J. Zhang, M. Zhang, P. Zhang, Q. Zhang, S. Zhang, S. Zhang, S. Zhang, S. Zhang, T. Zhang, X. Zhang, X. Zhang, X. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Y. Zhang, Z. Zhang, Z. Zhang, 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, K. Zhu, K. Zhu, Z. Zhu, B. Zhuang, H. Zhuang, L. Zong, J. Zou, J. Züfle, S. Zwickel. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2023:10(2023), pp. 022.1-022.39. [10.1088/1475-7516/2023/10/022]

JUNO sensitivity to 7Be, pep, and CNO solar neutrinos

Abusleme, Angel;Adam, Thomas;Ahmad, Shakeel;Ahmed, Rizwan;Aiello, Sebastiano;Akram, Muhammad;Aleem, Abid;Alexandros, Tsagkarakis;An, Fengpeng;An, Qi;Andronico, Giuseppe;Anfimov, Nikolay;Antonelli, Vito;Antoshkina, Tatiana;Asavapibhop, Burin;Auguste, Didier;Bai, Weidong;Balashov, Nikita;Baldini, Wander;Barresi, Andrea;D. Basilico;Baussan, Eric;Bellato, Marco;M. Beretta;Bergnoli, Antonio;Bick, Daniel;Bieger, Lukas;Biktemerova, Svetlana;Birkenfeld, Thilo;Blum, David;Blyth, Simon;Bolshakova, Anastasia;Bongrand, Mathieu;Bordereau, Clément;Breton, Dominique;Brigatti, Augusto;Brugnera, Riccardo;Bruno, Riccardo;Budano, Antonio;Busto, Jose;Cabrera, Anatael;Caccianiga, Barbara;Cai, Hao;Cai, Xiao;Cai, Yanke;Cai, Zhiyan;Callier, Stéphane;Cammi, Antonio;Campeny, Agustin;Cao, Chuanya;Cao, Guofu;Cao, Jun;Caruso, Rossella;Cerna, Cédric;Cerrone, Vanessa;Chan, Chi;Chang, Jinfan;Chang, Yun;Chen, Chao;Chen, Guoming;Chen, Pingping;Chen, Shaomin;Chen, Yixue;Chen, Yu;Chen, Zhiyuan;Chen, Zikang;Cheng, Jie;Cheng, Yaping;Cheng, Yu Chin;Chepurnov, Alexander;Chetverikov, Alexey;Chiesa, Davide;Chimenti, Pietro;Chu, Ziliang;Chukanov, Artem;Claverie, Gérard;Clementi, Catia;Clerbaux, Barbara;Molla, Marta Colomer;Lorenzo, Selma Conforti Di;Coppi, Alberto;Corti, Daniele;Csakli, Simon;Corso, Flavio Dal;Dalager, Olivia;Datta, Jaydeep;Taille, Christophe De La;Deng, Zhi;Deng, Ziyan;Depnering, Wilfried;Ding, Xiaoyu;Ding, Xuefeng;Ding, Yayun;Dirgantara, Bayu;Dittrich, Carsten;Dmitrievsky, Sergey;Dohnal, Tadeas;Dolzhikov, Dmitry;Donchenko, Georgy;Dong, Jianmeng;Doroshkevich, Evgeny;Dou, Wei;Dracos, Marcos;Druillole, Frédéric;Du, Ran;Du, Shuxian;Dugas, Katherine;Dusini, Stefano;Duyang, Hongyue;Eck, Jessica;Enqvist, Timo;Fabbri, Andrea;Fahrendholz, Ulrike;Fan, Lei;Fang, Jian;Fang, Wenxing;Fargetta, Marco;Fedoseev, Dmitry;Fei, Zhengyong;Feng, Li-Cheng;Feng, Qichun;Ferraro, Federico;Fournier, Amélie;Gan, Haonan;Gao, Feng;Garfagnini, Alberto;Gavrikov, Arsenii;Giammarchi, Marco;Giudice, Nunzio;Gonchar, Maxim;Gong, Guanghua;Gong, Hui;Gornushkin, Yuri;Göttel, Alexandre;Grassi, Marco;Gromov, Maxim;Gromov, Vasily;Gu, Minghao;Gu, Xiaofei;Gu, Yu;Guan, Mengyun;Guan, Yuduo;Guardone, Nunzio;Guo, Cong;Guo, Wanlei;Guo, Xinheng;Hagner, Caren;Han, Ran;Han, Yang;He, Miao;He, Wei;Heinz, Tobias;Hellmuth, Patrick;Heng, Yuekun;Herrera, Rafael;Hor, YuenKeung;Hou, Shaojing;Hsiung, Yee;Hu, Bei-Zhen;Hu, Hang;Hu, Jianrun;Hu, Jun;Hu, Shouyang;Hu, Tao;Hu, Yuxiang;Hu, Zhuojun;Huang, Guihong;Huang, Hanxiong;Huang, Jinhao;Huang, Junting;Huang, Kaixuan;Huang, Wenhao;Huang, Xin;Huang, Xingtao;Huang, Yongbo;Hui, Jiaqi;Huo, Lei;Huo, Wenju;Huss, Cédric;Hussain, Safeer;Imbert, Leonard;Ioannisian, Ara;Isocrate, Roberto;Jelmini, Beatrice;Jeria, Ignacio;Ji, Xiaolu;Jia, Huihui;Jia, Junji;Jian, Siyu;Jiang, Cailian;Jiang, Di;Jiang, Wei;Jiang, Xiaoshan;Jing, Xiaoping;Jollet, Cécile;Kampmann, Philipp;Kang, Li;Karaparambil, Rebin;Kazarian, Narine;Khan, Ali;Khatun, Amina;Khosonthongkee, Khanchai;Korablev, Denis;Kouzakov, Konstantin;Krasnoperov, Alexey;Kuleshov, Sergey;Kutovskiy, Nikolay;Lachenmaier, Tobias;Landini, Cecilia;Leblanc, Sébastien;Lebrin, Victor;Lefevre, Frederic;Lei, Ruiting;Leitner, Rupert;Leung, Jason;Li, Demin;Li, Fei;Li, Fule;Li, Gaosong;Li, Huiling;Li, Jiajun;Li, Mengzhao;Li, Min;Li, Nan;Li, Qingjiang;Li, Ruhui;Li, Rui;Li, Shanfeng;Li, Tao;Li, Teng;Li, Weidong;Li, Weiguo;Li, Xiaomei;Li, Xiaonan;Li, Xinglong;Li, Yi;Li, Yichen;Li, Yufeng;Li, Zepeng;Li, Zhaohan;Li, Zhibing;Li, Ziyuan;Li, Zonghai;Liang, Hao;Liang, Hao;Liao, Jiajun;Limphirat, Ayut;Lin, Guey-Lin;Lin, Shengxin;Lin, Tao;Ling, Jiajie;Ling, Xin;Lippi, Ivano;Liu, Caimei;Liu, Fang;Liu, Fengcheng;Liu, Haidong;Liu, Haotian;Liu, Hongbang;Liu, Hongjuan;Liu, Hongtao;Liu, Hui;Liu, Jianglai;Liu, Jiaxi;Liu, Jinchang;Liu, Min;Liu, Qian;Liu, Qin;Liu, Runxuan;Liu, Shenghui;Liu, Shubin;Liu, Shulin;Liu, Xiaowei;Liu, Xiwen;Liu, Xuewei;Liu, Yankai;Liu, Zhen;Lokhov, Alexey;Lombardi, Paolo;Lombardo, Claudio;Loo, Kai;Lu, Chuan;Lu, Haoqi;Lu, Jingbin;Lu, Junguang;Lu, Peizhi;Lu, Shuxiang;Lubsandorzhiev, Bayarto;Lubsandorzhiev, Sultim;Ludhova, Livia;Lukanov, Arslan;Luo, Daibin;Luo, Fengjiao;Luo, Guang;Luo, Jianyi;Luo, Shu;Luo, Wuming;Luo, Xiaojie;Lyashuk, Vladimir;Ma, Bangzheng;Ma, Bing;Ma, Qiumei;Ma, Si;Ma, Xiaoyan;Ma, Xubo;Maalmi, Jihane;Magoni, Marco;Mai, Jingyu;Malyshkin, Yury;Mandujano, Roberto Carlos;Mantovani, Fabio;Mao, Xin;Mao, Yajun;Mari, Stefano M.;Marini, Filippo;Martini, Agnese;Mayer, Matthias;Mayilyan, Davit;Mednieks, Ints;Meng, Yue;Meraviglia, Anita;Meregaglia, Anselmo;Meroni, Emanuela;Meyhöfer, David;L. 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2023

Abstract

The Jiangmen Underground Neutrino Observatory (JUNO), the first multi-kton liquid scintillator detector, which is under construction in China, will have a unique potential to perform a real-time measurement of solar neutrinos well below the few MeV threshold typical of Water Cherenkov detectors. JUNO's large target mass and excellent energy resolution are prerequisites for reaching unprecedented levels of precision. In this paper, we provide estimation of the JUNO sensitivity to 7Be, pep, and CNO solar neutrinos that can be obtained via a spectral analysis above the 0.45 MeV threshold. This study is performed assuming different scenarios of the liquid scintillator radiopurity, ranging from the most optimistic one corresponding to the radiopurity levels obtained by the Borexino experiment, up to the minimum requirements needed to perform the neutrino mass ordering determination with reactor antineutrinos — the main goal of JUNO. Our study shows that in most scenarios, JUNO will be able to improve the current best measurements on 7Be, pep, and CNO solar neutrino fluxes. We also perform a study on the JUNO capability to detect periodical time variations in the solar neutrino flux, such as the day-night modulation induced by neutrino flavor regeneration in Earth, and the modulations induced by temperature changes driven by helioseismic waves.

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	Settori scientifico-disciplinari dell'articolo
	
			Settore FIS/01 - Fisica Sperimentale
Settore FIS/04 - Fisica Nucleare e Subnucleare
		
	Data di pubblicazione
	
			2023
		
	Data ahead of print o data di stampa
	
			7-ott-2023
		
	Rivista in ANCE
	
			JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
		
	DOI
	
			https://dx.doi.org/10.1088/1475-7516/2023/10/022
		
	Tipologia
	
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			01 - Articolo su periodico

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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1008710

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