Abstract
Monte Carlo simulations were used to study the gamma-ray spectra of pebble bed reactor fuel at various levels of burnup. A fuel depletion calculation was performed using the ORIGEN2.1 code, which yielded the gamma-ray source term that was introduced into the input of an MCNP4C simulation. The simulation assumed the use of a 100% efficient high-purity coaxial germanium (HPGe) detector, a pebble placed at a distance of 100 cm from the detector, and accounted for Gaussian broadening of the gamma-ray peaks. Previously, it was shown that 137Cs, 60Co (introduced as a dopant), and 134Cs are the relevant burnup indicators. The results show that the 662keV line of 137Cs lies in close proximity to the intense 658keV of 197Nb, which results in spectral interference between the lines. However, the 1333keV line of 60Co, and selected 134Cs lines (e.g., at 605keV) are free from spectral interference, which enhances the possibility of their utilization as relative burnup indicators.
Original language | English (US) |
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Pages (from-to) | 393-396 |
Number of pages | 4 |
Journal | Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment |
Volume | 505 |
Issue number | 1-2 |
DOIs | |
State | Published - Jun 1 2003 |
Externally published | Yes |
Event | Proceedings of the tenth Symposium on Radiation - Ann Arbor, MI, United States Duration: May 21 2002 → May 23 2002 |
Keywords
- Burnup
- Fuel
- Gamma ray
- Germanium detector
- Monte Carlo
- Pebble bed reactor
- Spectrometry
ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Instrumentation