Improved Constraints on Sterile Neutrino Mixing from Disappearance Searches in the MINOS, 
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, Daya Bay, and Bugey-3 Experiments

Adamson, P.; An, Fengpeng; Anghel, I. M.; Aurisano, A.; Balantekin, A. B.; Band, H. R.; Barr, G.; Bishai, M.; Blake, A.; Blyth, S.; Cao, G. F.; Cao, Jun; Cao, S.; Carroll, Timothy J.; Castromonte, C.; Chang, J. F.; Chang, Yun Hsuan; Chen, H. S.; Chen, R.; Chen, S. M.; Chen, Y.; Chen, Y. X.; Cheng, Jie; Cheng, Z. K.; Cherwinka, J. J.; Childress, S.; Chu, M. C.; Chukanov, A.; Coelho, J. A. B.; Cummings, J. P.; Dash, N.; Rijck, S. De; Deng, F. S.; Ding, Yayun; Diwan, M. V.; Dohnal, Tadeáš; Dolzhikov, Dmitry; Dove, J.; Dvořák, Martin; Dwyer, D. A.; Evans, Justin J.; Feldman, G. J.; Flanagan, W.; Gabrielyan, M.; Gallo, J. P.; Germani, S.; Gomes, R. A.; Gonchar, M.; Gong, Guanghua; Gong, H.; Gouffon, P.; Graf, N.; Grzelak, K.; Gu, W.; Guo, Jingyuan; Guo, L.; Guo, X. H.; Guo, Yuhang; Guo, Ziyi; Habig, A.; Hackenburg, R.; Hahn, S. R.; Hans, S.; Hartnell, J.; Hatcher, R.; He, M.; Heeger, K. M.; Heng, Y. K.; Higuera, A.; Holin, A.; Hor, YuenKeung; Hsiung, Y.; Hu, Bei-Zhen; Hu, Jun; Hu, T.; Hu, Z. J.; Huang, Hanxiong; Huang, J.; Huang, X. T.; Huang, Yongbo; Huber, Patrick; Jaffe, D. E.; Jen, K. L.; Ji, X. L.; Ji, X.; Johnson, R. A.; Jones, D.; Li, Kang; Kettell, S. H.; Koerner, L. W.; Kohn, S.; Kordosky, M.; Krämer, M.; Kreymer, A.; Lang, K.; Langford, T.; Lee, J.; Lee, J. H. C.; Lei, Ruiting; Leitner, R.; Leung, J. K. C.; Li, F.; Li, H. L.; Li, J. J.; Li, Q. J.; Li, S.; Li, S. C.; Li, S. J.; Li, W. D.; Li, X. N.; Li, X. Q.; Li, Y. F.; Li, Z. B.; Liu, Han; Lin, C. J.; Lin, G. L.; Lin, Shengxin; Ling, Jiajie; Link, J. M.; Littenberg, L.; Littlejohn, B. R.; Liu, J. C.; Liu, J. L.; Liu, Y.; Liu, Y. H.; Lü, C.; Lu, Haoqi; Lu, J. S.; Lucas, P.; Luk, K. B.; B., X.; Y., X.; Q., Y.; Mann, W. A.; Маршак, М. Л.; Marshall, C.; Caicedo, D. A. Martínez; Mayer, N.; McDonald, Kirk T.; McKeown, R. D.; Mehdiyev, R.; Meier, J. R.; Meng, Y.; Miller, William H.; Mills, G. B.; Lepin, L. Mora; Naples, D.; Napolitano, J.; Naumov, D.; Наумова, Э.; Nelson, J. K.; Nichol, R. J.; O’Connor, J. Michael; Ochoa-Ricoux, J. P.; Olshevskiy, A.; Pahlka, R. B.; Pan, H.-R.; Park, J.; Patton, S.; Pavlović, Ž.; Pawloski, G.; Peng, J. C.; Perch, A.; Pfützner, M. M.; Phan, D. D.; Plunkett, R.; Poonthottathil, N.; Pun, C. S. J.; Qi, F. Z.; Qi, M.; Qian, X.; Qiu, X.; Radovic, A.; Raper, N.; Ren, Jie; Reveco, C. Morales; Rosero, R.; Roskovec, B.; Ruan, Xichao; Sail, P.; Sanchez, M. C.; Schneps, J.; Schreckenberger, A.; Shaheed, Nasir; Sharma, R.; Sousa, A.; Steiner, H.; Sun, Jian; Tagg, N.; Thomas, J.; Thomson, M.; Timmons, A.; Tměj, Tomáš; Todd, J.; Tognini, S. C.; Toner, R.; Torretta, D.; Treskov, Konstantin; Tse, W.-H.; Tull, C. E.; Vahle, P.; Viren, B.; Vorobel, V.; Wang, C. H.; Wang, J.; Wang, M.; Wang, N. Y.; Wang, R. G.; Wang, W.; Wang, X.; Wang, Y.; Wang, Y. F.; Wang, Z.; Wang, Z. M.; Weber, A.; Wei, H.; Wei, Lianghong; Wen, L.; Whisnant, K.; White, C.; Whitehead, L.; Wojcicki, S. G.; Wong, H. L. H.; Wong, Steven Chan-Fai; Worcester, E.; Wu, Diru; Wu, Fangliang; Wu, Qun; Wu, W.; Xia, Dongmei; Xie, Z.; Xing, Zhi-zhong; Jinsong, Xu; Xu, T.; Xue, T.; Yang, Changgen; Yang, Lei; Yang, Yifan; Yao, Haifeng; Ye, M.; Yeh, M.; Young, Ben; Yu, Hongzhao; Yu, Zezhong; Yue, Baobiao; Zeng, S.; Zeng, Yuda; Zhan, Liang; Zhang, C.; Zhang, F. Y.; Zhang, H. H.; Zhang, J. W.; Zhang, Q. M.; Zhang, X. T.; Zhang, Y. M.; Zhang, Y. X.; Zhang, Y. Y.; Zhang, Z. J.; Zhang, Z. P.; Zhang, Z. Y.; Zhao, J.; Li, Zhou; Zhuang, H. L.; Mo, Mo; mrow,

doi:10.1103/physrevlett.125.071801

Cited by 68 publications

(74 citation statements)

References 57 publications

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“…Several experimental hints point towards the existence of sterile neutrinos, which have been extensively investigated in many experiments. The possible observation of short baseline oscillations in some of these experiments [266][267][268][269][270][271][272][273] together with the non-observation of neutrino oscillations in others [23,[274][275][276][277][278][279][280][281][282][283] lead to large tensions in the global 3+1 picture [284][285][286][287][288]. Even though there is some theoretical overlap, these results would point towards new mass splittings at the ∼ 1 eV 2 scale.…”

Section: Introductionmentioning

confidence: 98%

Neutrino oscillation phenomenology in the standard model and beyond

Ternes

2020

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Section: Introductionmentioning

confidence: 98%

Neutrino oscillation phenomenology in the standard model and beyond

Ternes

2020

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“…The Daya Bay reactor neutrino experiment started data taking on December 24, 2011. With millions of ν e interactions detected in eight identically designed ADs in three underground EHs, many physics results have been produced, including the current world-leading measurements of the neutrino mixing angle θ 13 and the squared masssplitting |∆m 2 32 | [16], precise measurements of the reactor ν e flux and spectrum [17,18,19], and stringent limits on the existence of light sterile neutrinos [20,21]. Three nested cylindrical volumes in each AD are separated by concentric acrylic vessels (IAV, OAV), as shown in Fig.…”

Section: The Juno Ls Pilot Experiments At Daya Baymentioning

confidence: 99%

Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector

Abusleme

Adam

Ahmad

et al. 2021

Nuclear Instruments and Methods in Physics Research Section A:

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This is a PDF file of an article that has undergone enhancements after acceptance, such as the addition of a cover page and metadata, and formatting for readability, but it is not yet the definitive version of record. This version will undergo additional copyediting, typesetting and review before it is published in its final form, but we are providing this version to give early visibility of the article. Please note that, during the production process, errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.

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“…The ORCA sensitivity is compared with upper limits from cosmology [13] for which only 95% C.L. are available, and upper limits from MINOS/MINOS+ [44], IceCube [45] and SK [42]. The obtained sensitivity is compared with current upper limits from cosmology [13], MINOS/MINOS+ [44], IceCube (IC) [45] and SK [42].…”

Section: Sensitivity To θ 24 For Different ∆M 2 41 Valuesmentioning

confidence: 99%

“…are available, and upper limits from MINOS/MINOS+ [44], IceCube [45] and SK [42]. The obtained sensitivity is compared with current upper limits from cosmology [13], MINOS/MINOS+ [44], IceCube (IC) [45] and SK [42]. The excluded region is the one on the right of the lines, for IceCube at 90% C.L.…”

Section: Sensitivity To θ 24 For Different ∆M 2 41 Valuesmentioning

confidence: 99%

Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

Aiello

López

Díaz

et al. 2021

J. High Energ. Phys.

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KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles θ14, θ24, θ34 and the effective angle θμe, over a broad range of mass squared difference $$ \Delta {m}_{41}^2 $$ ∆ m 41 2 ∼ [10−5, 10] eV2, allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.

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Improved Constraints on Sterile Neutrino Mixing from Disappearance Searches in the MINOS, MINOS+ , Daya Bay, and Bugey-3 Experiments

Cited by 68 publications

References 57 publications

Neutrino oscillation phenomenology in the standard model and beyond

Neutrino oscillation phenomenology in the standard model and beyond

Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector

Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

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