The neutron flux at a depth of 850 m.w.e., according to BUST data
- 作者: Boliev M.M.1, Volchenko V.I.1, Volchenko V.G.1, Dzaparova I.M.1,2, Kochkarov M.M.1, Novoseltsev Y.F.1, Novoseltseva R.V.1, Petkov V.B.1,2, Yanin A.F.1
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隶属关系:
- Institute for Nuclear Research
- Institute of Astronomy
- 期: 卷 81, 编号 4 (2017)
- 页面: 509-511
- 栏目: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185057
- DOI: https://doi.org/10.3103/S1062873817040104
- ID: 185057
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详细
A way of estimating a muon-enduced neutron flux has been proposed. The technique is used to estimate the neutron background at the Baksan Underground Scintillation Telescope (BUST). A two-pulse signature (unstable 12B production and its subsequent decay) is used to identify neutron events. The integrated average neutron flux on the external planes of detector is an order of magnitude higher than the one on the internal planes. Within the limits of statistical error, the resulting neutron flux agrees with predictions from simulations for the depth at which the BUST lies using the FLUKA program.
作者简介
M. Boliev
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
V. Volchenko
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
V. Volchenko
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
I. Dzaparova
Institute for Nuclear Research; Institute of Astronomy
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312; Moscow, 119017
M. Kochkarov
Institute for Nuclear Research
编辑信件的主要联系方式.
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
Yu. Novoseltsev
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
R. Novoseltseva
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
V. Petkov
Institute for Nuclear Research; Institute of Astronomy
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312; Moscow, 119017
A. Yanin
Institute for Nuclear Research
Email: kchkrv@rambler.ru
俄罗斯联邦, Moscow, 117312
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