Cargando…

Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND

PURPOSE: Monte Carlo (MC) modelling techniques have been used extensively in Nuclear Medicine (NM). The theoretical energy resolution relationship ([Formula: see text]), does not accurately predict the gamma camera detector response across all energies. This study aimed to validate the accuracy of a...

Descripción completa

Detalles Bibliográficos
Autores principales: Morphis, Michaella, van Staden, Johan A., du Raan, Hanlie, Ljungberg, Michael
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7892923/
https://www.ncbi.nlm.nih.gov/pubmed/33659726
http://dx.doi.org/10.1016/j.heliyon.2021.e06097
_version_ 1783652953022791680
author Morphis, Michaella
van Staden, Johan A.
du Raan, Hanlie
Ljungberg, Michael
author_facet Morphis, Michaella
van Staden, Johan A.
du Raan, Hanlie
Ljungberg, Michael
author_sort Morphis, Michaella
collection PubMed
description PURPOSE: Monte Carlo (MC) modelling techniques have been used extensively in Nuclear Medicine (NM). The theoretical energy resolution relationship ([Formula: see text]), does not accurately predict the gamma camera detector response across all energies. This study aimed to validate the accuracy of an energy resolution model for the SIMIND MC simulation code emulating the Siemens Symbia T16 dual-head gamma camera. METHODS: Measured intrinsic energy resolution data (full width half maximum (FWHM) values), for Ba-133, Lu-177, Am-241, Ga-67, Tc-99m, I-123, I-131 and F-18 sources in air, were used to create a fitted model of the energy response of the gamma camera. Both the fitted and theoretical models were used to simulate intrinsic and extrinsic energy spectra using three different scenarios (source in air; source in simple scatter phantom and a clinical voxel-based digital patient phantom). RESULTS: The results showed the theoretical model underestimated the FWHM values at energies above 160.0 keV up to 23.5 keV. In contrast, the fitted model better predicted the measured FWHM values with differences less than 3.3 keV. The I-131 in-scatter energy spectrum simulated with the fitted model better matched the measured energy spectrum. Higher energy photopeaks, (I-123: 528.9 keV and I-131: 636.9 keV) simulated with the fitted model, more accurately resembled the measured photopeaks. The voxel-based digital patient phantom energy spectra, simulated with the fitted and theoretical models, showed the potential impact of an incorrect energy resolution model when simulating isotopes with multiple photopeaks. CONCLUSION: Modelling of energy resolution with the proposed fitted model enables the SIMIND user to accurately simulate NM images. A great improvement was seen for high-energy photon emitting isotopes (e.g. I-131), as well as isotopes with multiple photopeaks (e.g. Lu-177, I-131 and Ga-67) in comparison to the theoretical model. This will result in accurate evaluation of radioactivity quantification, which is vital for dosimetric purposes.
format Online
Article
Text
id pubmed-7892923
institution National Center for Biotechnology Information
language English
publishDate 2021
publisher Elsevier
record_format MEDLINE/PubMed
spelling pubmed-78929232021-03-02 Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND Morphis, Michaella van Staden, Johan A. du Raan, Hanlie Ljungberg, Michael Heliyon Research Article PURPOSE: Monte Carlo (MC) modelling techniques have been used extensively in Nuclear Medicine (NM). The theoretical energy resolution relationship ([Formula: see text]), does not accurately predict the gamma camera detector response across all energies. This study aimed to validate the accuracy of an energy resolution model for the SIMIND MC simulation code emulating the Siemens Symbia T16 dual-head gamma camera. METHODS: Measured intrinsic energy resolution data (full width half maximum (FWHM) values), for Ba-133, Lu-177, Am-241, Ga-67, Tc-99m, I-123, I-131 and F-18 sources in air, were used to create a fitted model of the energy response of the gamma camera. Both the fitted and theoretical models were used to simulate intrinsic and extrinsic energy spectra using three different scenarios (source in air; source in simple scatter phantom and a clinical voxel-based digital patient phantom). RESULTS: The results showed the theoretical model underestimated the FWHM values at energies above 160.0 keV up to 23.5 keV. In contrast, the fitted model better predicted the measured FWHM values with differences less than 3.3 keV. The I-131 in-scatter energy spectrum simulated with the fitted model better matched the measured energy spectrum. Higher energy photopeaks, (I-123: 528.9 keV and I-131: 636.9 keV) simulated with the fitted model, more accurately resembled the measured photopeaks. The voxel-based digital patient phantom energy spectra, simulated with the fitted and theoretical models, showed the potential impact of an incorrect energy resolution model when simulating isotopes with multiple photopeaks. CONCLUSION: Modelling of energy resolution with the proposed fitted model enables the SIMIND user to accurately simulate NM images. A great improvement was seen for high-energy photon emitting isotopes (e.g. I-131), as well as isotopes with multiple photopeaks (e.g. Lu-177, I-131 and Ga-67) in comparison to the theoretical model. This will result in accurate evaluation of radioactivity quantification, which is vital for dosimetric purposes. Elsevier 2021-02-10 /pmc/articles/PMC7892923/ /pubmed/33659726 http://dx.doi.org/10.1016/j.heliyon.2021.e06097 Text en © 2021 Published by Elsevier Ltd. http://creativecommons.org/licenses/by-nc-nd/4.0/ This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
spellingShingle Research Article
Morphis, Michaella
van Staden, Johan A.
du Raan, Hanlie
Ljungberg, Michael
Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title_full Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title_fullStr Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title_full_unstemmed Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title_short Modelling of energy-dependent spectral resolution for SPECT Monte Carlo simulations using SIMIND
title_sort modelling of energy-dependent spectral resolution for spect monte carlo simulations using simind
topic Research Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7892923/
https://www.ncbi.nlm.nih.gov/pubmed/33659726
http://dx.doi.org/10.1016/j.heliyon.2021.e06097
work_keys_str_mv AT morphismichaella modellingofenergydependentspectralresolutionforspectmontecarlosimulationsusingsimind
AT vanstadenjohana modellingofenergydependentspectralresolutionforspectmontecarlosimulationsusingsimind
AT duraanhanlie modellingofenergydependentspectralresolutionforspectmontecarlosimulationsusingsimind
AT ljungbergmichael modellingofenergydependentspectralresolutionforspectmontecarlosimulationsusingsimind