| 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; 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| 2022
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Source Publication | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
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Issue | 10 |
Subtype | Article
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Abstract | We 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. |
Keyword | neutrino astronomy
neutrino detectors
supernova neutrinos
diffuse supernova neutrino background
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DOI | 10.1088/1475-7516/2022/10/033
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Indexed By | ADS
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Language | 英语
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WOS ID | WOS:000928487200025
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ADS Bibcode | 2022JCAP...10..033A
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ADS URL | https://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A
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ADS CITATIONS | https://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A/citations
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Citation statistics |
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Document Type | 期刊论文
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Identifier | http://ir.ihep.ac.cn/handle/311005/297546
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Collection | 江门中微子实验
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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).
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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).
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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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