Numerical Simulation of Radiation Anisotropy of the Pyroelectric Neutron Generator
- Autores: Gromov M.B.1, Kubankin A.S.2,3, Ionidi V.Y.1, Kaplii A.A.2, Kirsanov M.A.4, Klenin A.A.2, Kolesnikov D.A.2,5, Oleinik A.N.2,6, Chepurnov A.S.1, Shchagin A.V.2,5
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Afiliações:
- Skobeltsyn Institute of Nuclear Physics
- Laboratory of Radiation Physics
- Lebedev Physical Institute
- Moscow Engineering Physics Institute
- Kharkiv Institute of Physics and Technology
- John Adams Institute at Royal Holloway
- Edição: Volume 74, Nº 2 (2019)
- Páginas: 144-148
- Seção: The Physics of the Atomic Nucleus and Elementary Particles
- URL: https://journals.rcsi.science/0027-1349/article/view/165095
- DOI: https://doi.org/10.3103/S0027134919020085
- ID: 165095
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Resumo
The pyroelectric neutron generator is a compact source of fast neutrons with an energy of 2.45 MeV and a yield up to ∼104 neutrons/s. The device is designed for calibration of low-background neutrino and dark matter detectors and may also serve as an alternative to traditional radioactive sources of fast neutrons in physical research and practical work. Numerical simulation of the angular distribution of neutrons emitted by the pyroelectric generator with the D(d, n)3He reaction proceeding within it was performed in order to calculate the neutron yield in the full solid angle and in a given direction correctly. The angular distribution was found to be anisotropic: the neutron yield increased in the direction of motion of incident deuterium ions. This anisotropy was as large as ∼25% at a maximum energy of 28 keV of incident particles. The anisotropy increased nonlinearly with the ion energy: it reached ∼70% at 50 keV and a monoenergetic flux, but was virtually zero below 10 keV. The obtained angular distribution is similar to that of neutrons in the case of a 15-keV monoenergetic flux of deuterium ions.
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Sobre autores
M. Gromov
Skobeltsyn Institute of Nuclear Physics
Autor responsável pela correspondência
Email: gromov@physics.msu.ru
Rússia, Moscow, 119234
A. Kubankin
Laboratory of Radiation Physics; Lebedev Physical Institute
Autor responsável pela correspondência
Email: askubankin@gmail.com
Rússia, Belgorod, 308034; Moscow, 119333
V. Ionidi
Skobeltsyn Institute of Nuclear Physics
Email: askubankin@gmail.com
Rússia, Moscow, 119234
A. Kaplii
Laboratory of Radiation Physics
Email: askubankin@gmail.com
Rússia, Belgorod, 308034
M. Kirsanov
Moscow Engineering Physics Institute
Email: askubankin@gmail.com
Rússia, Moscow, 115409
A. Klenin
Laboratory of Radiation Physics
Email: askubankin@gmail.com
Rússia, Belgorod, 308034
D. Kolesnikov
Laboratory of Radiation Physics; Kharkiv Institute of Physics and Technology
Email: askubankin@gmail.com
Rússia, Belgorod, 308034; Kharkiv, 61108
A. Oleinik
Laboratory of Radiation Physics; John Adams Institute at Royal Holloway
Email: askubankin@gmail.com
Rússia, Belgorod, 308034; Egham, Surrey, TW20 0EX
A. Chepurnov
Skobeltsyn Institute of Nuclear Physics
Email: askubankin@gmail.com
Rússia, Moscow, 119234
A. Shchagin
Laboratory of Radiation Physics; Kharkiv Institute of Physics and Technology
Email: askubankin@gmail.com
Rússia, Belgorod, 308034; Kharkiv, 61108
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