Spectral Discrimination of Deposited Gamma-Ray Energies in a Simulated CeBr3 Scintillator
Abstract
We show that wavelength measurements of individual detected optical photons may provide additional information about gamma-ray energy deposited in a CeBr3 crystal when the detected-photon-count distributions overlap for nearby gamma-ray energies. Monoenergetic 662 and 629 keV gammas are used in a Geant4 simulation of a 25×25×20 mm3 CeBr3 crystal. Assuming a light yield of 6.0×104 photons/MeV, a wavelength-independent photon-detection efficiency of 30%, and a wavelength resolution of σλ=40 nm, we find that the fraction of photons reconstructed above 385 nm gives an event-level separation of ∼ 2 standard deviations between the 662 and 629 keV event populations selected within the same ∼ 1%-wide detected-photon-count interval. No timing or reconstructed interaction-position information is used. The result demonstrates, within the present simulation model, that event-dependent optical spectra can retain energy information beyond an undifferentiated photon count.
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BibTeX
@misc{elagin2026spectral,
title = {{Spectral Discrimination of Deposited Gamma-Ray Energies in a Simulated CeBr$_3$ Scintillator}},
author = {Andrey Elagin},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.09640},
eprint = {2609.09640},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.09640},
}
RIS
TY - UNPB
TI - Spectral Discrimination of Deposited Gamma-Ray Energies in a Simulated CeBr_3 Scintillator
AU - Andrey Elagin
PY - 2026
DA - 2026/09/09
PB - arXiv
DO - 10.48550/arxiv.2609.09640
UR - https://arxiv.org/abs/2609.09640
AB - We show that wavelength measurements of individual detected optical photons may provide additional information about gamma-ray energy deposited in a CeBr_3 crystal when the detected-photon-count distributions overlap for nearby gamma-ray energies. Monoenergetic 662 and 629 keV gammas are used in a Geant4 simulation of a 25×25×20 mm^3 CeBr_3 crystal. Assuming a light yield of 6.0×10^4 photons/MeV, a wavelength-independent photon-detection efficiency of 30%, and a wavelength resolution of σ_λ=40 nm, we find that the fraction of photons reconstructed above 385 nm gives an event-level separation of ∼ 2 standard deviations between the 662 and 629 keV event populations selected within the same ∼ 1%-wide detected-photon-count interval. No timing or reconstructed interaction-position information is used. The result demonstrates, within the present simulation model, that event-dependent optical spectra can retain energy information beyond an undifferentiated photon count.
ER -