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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Main Authors: Gennady N. Vlaskin, Sergey V. Bedenko, Nima Ghal-Eh, Hector R. Vega-Carrillo
Format: Article
Language:English
Published: Elsevier 2021-12-01
Series:Nuclear Engineering and Technology
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S1738573321003442
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spelling 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
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