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	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 Publication	JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Issue	10
Subtype	Article
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
DOI	10.1088/1475-7516/2022/10/033
Indexed By	ADS
Language	英语
WOS ID	WOS:000928487200025
ADS Bibcode	2022JCAP...10..033A
ADS URL	https://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A
ADS CITATIONS	https://ui.adsabs.harvard.edu/abs/2022JCAP...10..033A/citations
Citation statistics	Cited Times:12 [ADS]
Document Type	期刊论文
Identifier	http://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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