Seasonal variations in the muon-induced neutron flux and background of natural radioactivity at the Gran Sasso Underground Laboratory

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Cosmic ray muons at average energies of 280 GeV and muon-induced neutrons are detected by the LVD (Large Volume Detector). An analysis of seasonal variations in the neutron flux, based on data collected over 15 years, is presented. Measuring of the seasonal variations in the specific number of neutrons generated by muons allows us to determine the magnitude of variations in the average energy of the muon flux at the depth of the LVD’s location. The source of the seasonal variations in the total neutron flux is a change in the intensity and average energy of the muon flux. An analysis of the long-term monitoring of the LVD’s low-energy background is also presented.

作者简介

N. Agafonova

Institute for Nuclear Research

编辑信件的主要联系方式.
Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

V. Ashikhmin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

V. Dadykin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

E. Dobrynina

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

R. Enikeev

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

A. Malgin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

O. Ryazhskaya

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

I. Shakyrianova

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

V. Yakushev

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

Institute for Nuclear Research

Email: Natagafonova@gmail.com
俄罗斯联邦, Moscow, 117312

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