Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation
The 13C (α,n)16O reaction cross-section is important data for nuclear physics, astrophysical, and neutrino physics experiments, however, they exhibit uncertainties due to the discrepancies in the experimental data. In this study, using the Nedis-2m program code, the energy spectrum of α-induced neut...
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doaj-090961ab02f243c2b8f274c34642e1912021-09-17T04:34:29ZengElsevierNuclear Engineering and Technology1738-57332021-12-01531240674071Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulationGennady N. Vlaskin0Sergey V. Bedenko1Nima Ghal-Eh2Hector R. Vega-Carrillo3Innovation Technology Centre for the PRORYV Project, Rosatom, Moscow, RussiaSchool of Nuclear Science and Engineering, Tomsk Polytechnic University, Tomsk, Russia; Corresponding author.Department of Physics, Faculty of Science, Ferdowsi University of Mashhad, Mashhad, IranAcademic Unit of Nuclear Studies of the Autonomous University of Zacatecas, Zac., MexicoThe 13C (α,n)16O reaction cross-section is important data for nuclear physics, astrophysical, and neutrino physics experiments, however, they exhibit uncertainties due to the discrepancies in the experimental data. In this study, using the Nedis-2m program code, the energy spectrum of α-induced neutrons in a thin carbon target was calculated and the corresponding reaction cross-section was refined in the alpha particle energy range of 5–8 MeV. The results were used to calculate the intensity and energy spectrum of background neutrons produced in the liquid scintillator of KamLAND. The results will be useful in a variety of astrophysical and neutrino experiments especially those based on LS or Gd-LS detectors.http://www.sciencedirect.com/science/article/pii/S1738573321003442KamLAND13C(α,n)16O reaction cross sectionNeutron energy spectrumNedis-2m program Code |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Gennady N. Vlaskin Sergey V. Bedenko Nima Ghal-Eh Hector R. Vega-Carrillo |
spellingShingle |
Gennady N. Vlaskin Sergey V. Bedenko Nima Ghal-Eh Hector R. Vega-Carrillo Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation Nuclear Engineering and Technology KamLAND 13C(α,n)16O reaction cross section Neutron energy spectrum Nedis-2m program Code |
author_facet |
Gennady N. Vlaskin Sergey V. Bedenko Nima Ghal-Eh Hector R. Vega-Carrillo |
author_sort |
Gennady N. Vlaskin |
title |
Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation |
title_short |
Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation |
title_full |
Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation |
title_fullStr |
Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation |
title_full_unstemmed |
Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation |
title_sort |
neutron yield and energy spectrum of 13c(alpha,n)16o reaction in liquid scintillator of kamland: a nedis-2m simulation |
publisher |
Elsevier |
series |
Nuclear Engineering and Technology |
issn |
1738-5733 |
publishDate |
2021-12-01 |
description |
The 13C (α,n)16O reaction cross-section is important data for nuclear physics, astrophysical, and neutrino physics experiments, however, they exhibit uncertainties due to the discrepancies in the experimental data. In this study, using the Nedis-2m program code, the energy spectrum of α-induced neutrons in a thin carbon target was calculated and the corresponding reaction cross-section was refined in the alpha particle energy range of 5–8 MeV. The results were used to calculate the intensity and energy spectrum of background neutrons produced in the liquid scintillator of KamLAND. The results will be useful in a variety of astrophysical and neutrino experiments especially those based on LS or Gd-LS detectors. |
topic |
KamLAND 13C(α,n)16O reaction cross section Neutron energy spectrum Nedis-2m program Code |
url |
http://www.sciencedirect.com/science/article/pii/S1738573321003442 |
work_keys_str_mv |
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