Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation; Nuclear Engineering and Technology; Vol. 53, iss. 12

Dades bibliogràfiques
Parent link:Nuclear Engineering and Technology
Vol. 53, iss. 12.— 2021.— [P. 4067-4071]
Autor corporatiu: Национальный исследовательский Томский политехнический университет Инженерная школа ядерных технологий Отделение ядерно-топливного цикла
Altres autors: Vlaskin G. N. Gennadiy Nikolaevich, Bedenko S. V. Sergey Vladimirovich, Ghal-Eh N. Nima, Vega-Carrillo H. R. Hector Rene
Sumari:Title screen
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.
Idioma:anglès
Publicat: 2021
Matèries:
Accés en línia:https://doi.org/10.1016/j.net.2021.06.023
Format: MixedMaterials Electrònic Capítol de llibre
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=665467

MARC

LEADER 00000naa0a2200000 4500
001 665467
005 20250203164243.0
035 |a (RuTPU)RU\TPU\network\36666 
035 |a RU\TPU\network\35984 
090 |a 665467 
100 |a 20211007d2021 k||y0rusy50 ba 
101 0 |a eng 
102 |a NL 
135 |a drnn ---uucaa 
181 0 |a i  
182 0 |a b 
200 1 |a Neutron yield and energy spectrum of 13C(alpha,n)16O reaction in liquid scintillator of KamLAND: A Nedis-2m simulation  |f G. N. Vlaskin, S. V. Bedenko, N. Ghal-Eh, H. R. Vega-Carrillo  
203 |a Text  |c electronic 
300 |a Title screen 
320 |a [References: 23 tit.] 
330 |a 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. 
461 |t Nuclear Engineering and Technology 
463 |t Vol. 53, iss. 12  |v [P. 4067-4071]  |d 2021 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
610 1 |a KamLAND 
610 1 |a 13C(a,n)16O reaction cross section 
610 1 |a neutron energy spectrum 
610 1 |a nedis-2m program Code 
701 1 |a Vlaskin  |b G. N.  |g Gennadiy Nikolaevich 
701 1 |a Bedenko  |b S. V.  |c physicist  |c Associate Professor of Tomsk Polytechnic University, Candidate of physical and mathematical sciences  |f 1980-  |g Sergey Vladimirovich  |3 (RuTPU)RU\TPU\pers\30831  |9 15078 
701 1 |a Ghal-Eh  |b N.  |g Nima 
701 1 |a Vega-Carrillo  |b H. R.  |g Hector Rene 
712 0 2 |a Национальный исследовательский Томский политехнический университет  |b Инженерная школа ядерных технологий  |b Отделение ядерно-топливного цикла  |3 (RuTPU)RU\TPU\col\23554 
801 2 |a RU  |b 63413507  |c 20211007  |g RCR 
856 4 |u https://doi.org/10.1016/j.net.2021.06.023 
942 |c CF