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

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Аннотация

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.

Авторлар туралы

N. Agafonova

Institute for Nuclear Research

Хат алмасуға жауапты Автор.
Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

V. Ashikhmin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

V. Dadykin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

E. Dobrynina

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

R. Enikeev

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

A. Malgin

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

O. Ryazhskaya

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

I. Shakyrianova

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

V. Yakushev

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

Institute for Nuclear Research

Email: Natagafonova@gmail.com
Ресей, Moscow, 117312

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© Allerton Press, Inc., 2017