Published June 2018 | Version v1
Journal article

Monte Carlo simulation of tritium beta-ray induced X-ray spectrum in various gases

  • 1. Hydrogen Isotope Research Center, Organization for Promotion of Research, University of Toyama, 3190 Gofuku, Toyama City, Toyama 930-8555 (Japan)
  • 2. Electronics and Computer Engineering, National Institute of Technology, Toyama College, 1-2 Ebie-neriya, Imizu City, Toyama 933-0293 (Japan)
  • 3. KAKEN Company Limited, 1044 Horimachi, Mito City, Ibaraki 310-0903 (Japan)

Description

Highlights: • The beta-ray induced X-ray spectrometry (BIXS) is a gaseous tritium analysis method. • The gas medium dependence in BIXS was considered by Monte Carlo simulations. • The gas medium dependence in BIXS at low pressure was not serious issue. • The counting efficiency was enhanced by argon medium. - Abstract: Tritium beta-ray induced X-ray spectra in various gas mediums were simulated by Monte Carlo simulation using Geant4 tool kit. The simulated beta-ray induced X-ray spectrum (s-BIX spectrum) was composed of the bremsstrahlung component and characteristics X-rays from constituent elements. The total number of photons in s-BIX spectrum decreased with increasing pressure of medium except argon. In argon medium, the characteristics X-ray of argon was generated by beta particles from tritium decay, and the contribution of Ar-Kα and -Kβ compensated the reduction of bremsstrahlung generated by solid matter with increasing argon pressure. At 0.001 atm of medium pressure, the total counts in s-BIX spectrum was independent from gas medium. Therefore, the gas medium dependence in BIXS at low pressure (less than 0.001 atm) was not serious issue.

Availability note (English)

Available from http://dx.doi.org/10.1016/j.fusengdes.2018.04.080

Additional details

Identifiers

DOI
10.1016/j.fusengdes.2018.04.080;
PII
S0920379618303685;

Publishing Information

Journal Title
Fusion Engineering and Design
Journal Volume
131
Journal Page Range
p. 125-129
ISSN
0920-3796
CODEN
FEDEEE

Optional Information

Notes
© 2018 Elsevier B.V. All rights reserved.