IHEP OpenIR  > 江门中微子实验
Prospects for detecting the diffuse supernova neutrino background with JUNO
Abusleme, A; Adam, T; Ahmad, S; Ahmed, R; Aiello, S; Akram, M; An, FP; An, Q; Andronico, G; Anfimov, N; Antonelli, V; Antoshkina, T; Asavapibhop, B; de Andre, JPAM; Auguste, D; Balashov, N; Baldini, W; Barresi, A; Basilico, D; Baussan, E; Bellato, M; Bergnoli, A; Birkenfeld, T; Blin, S; Blum, D; Blyth, S; Bolshakova, A; Bongrand, M; Bordereau, C; Breton, D; Brigatti, A; Brugnera, R; Bruno, R; Budano, A; Buscemi, M; Busto, J; Butorov, I; Cabrera, A; Caccianiga, B; Cai, H; Cai, X; Cai, YK; Cai, ZY; Callegari, R; Cammi, A; Campeny, A; Cao, CY; Cao, GF; Cao, J; Caruso, R; Cerna, C; Chang, JF; Chang, Y; Chen, PP; Chen, PA; Chen, SM; Chen, XR; Chen, YW; Chen, YX; Chen, Y; Chen, Z; Cheng, J; Cheng, YP; Chetverikov, A; Chiesa, D; Chimenti, P; Chukanov, A; Claverie, G; Clementi, C; Clerbaux, B; Di Lorenzo, SC; Corti, D; Dal Corso, F; Dalager, O; De La Taille, C; Deng, Z; Deng, ZY; Depnering, W; Diaz, M; Ding, XF; Ding, YY; Dirgantara, B; Dmitrievsky, S; Dohnal, T; Dolzhikov, D; Donchenko, G; Dong, JM; 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Zhang, YH; Zhang, YY; Zhang, YP; Zhang, Y; Zhang, YY; Zhang, YM; Zhang, ZY; Zhang, ZJ; Zhao, FY; Zhao, J; Zhao, R; Zhao, SJ; Zhao, TC; Zheng, DQ; Zheng, H; Zheng, YH; Zhong, WR; Zhou, J; Zhou, L; Zhou, N; Zhou, S; Zhou, T; Zhou, X; Zhu, J; Zhu, KF; Zhu, KJ; Zhu, ZH; Zhuang, B; Zhuang, HL; Zong, L; Zou, JH
2022
Source PublicationJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Issue10
SubtypeArticle
AbstractWe present the detection potential for the diffuse supernova neutrino background (DSNB) at the Jiangmen Underground Neutrino Observatory (JUNO), using the inverse-beta-decay (IBD) detection channel on free protons. We employ the latest information on the DSNB flux predictions, and investigate in detail the background and its reduction for the DSNB search at JUNO. The atmospheric neutrino induced neutral current (NC) background turns out to be the most critical background, whose uncertainty is carefully evaluated from both the spread of model predictions and an envisaged in situ measurement. We also make a careful study on the background suppression with the pulse shape discrimination (PSD) and triple coincidence (TC) cuts. With latest DSNB signal predictions, more realistic background evaluation and PSD efficiency optimization, and additional TC cut, JUNO can reach the significance of 3 sigma for 3 years of data taking, and achieve better than 5 sigma after 10 years for a reference DSNB model. In the pessimistic scenario of non-observation, JUNO would strongly improve the limits and exclude a significant region of the model parameter space.
Keywordneutrino astronomy neutrino detectors supernova neutrinos diffuse supernova neutrino background
DOI10.1088/1475-7516/2022/10/033
Indexed ByADS
Language英语
WOS IDWOS:000928487200025
ADS Bibcode2022JCAP...10..033A
ADS URLhttps://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A
ADS CITATIONShttps://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A/citations
Citation statistics
Cited Times:12 [ADS]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/297546
Collection江门中微子实验
Recommended Citation
GB/T 7714
Abusleme, A,Adam, T,Ahmad, S,et al. Prospects for detecting the diffuse supernova neutrino background with JUNO[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2022(10).
APA Abusleme, A.,Adam, T.,Ahmad, S.,Ahmed, R.,Aiello, S.,...&Zou, JH.(2022).Prospects for detecting the diffuse supernova neutrino background with JUNO.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(10).
MLA Abusleme, A,et al."Prospects for detecting the diffuse supernova neutrino background with JUNO".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS .10(2022).
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