The neutron flux at a depth of 850 m.w.e., according to BUST data

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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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