Determining optimization of the initial parameters in Monte Carlo simulation for linear accelerator radiotherapy

Monte Carlo (MC) method is a well known calculation algorithm which can accurately assess the dose distribution for radiotherapy. The present study investigated all the possible regions of the depth-dose or lateral profiles which may affect the fitting of the initial parameters (mean energy and the...

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Veröffentlicht in:Radiation physics and chemistry (Oxford, England : 1993) England : 1993), 2014-02, Vol.95, p.161-165
Hauptverfasser: Chang, Kwo-Ping, Wang, Zhi-Wei, Shiau, An-Cheng
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Sprache:eng
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Zusammenfassung:Monte Carlo (MC) method is a well known calculation algorithm which can accurately assess the dose distribution for radiotherapy. The present study investigated all the possible regions of the depth-dose or lateral profiles which may affect the fitting of the initial parameters (mean energy and the radial intensity (full width at half maximum, FWHM) of the incident electron). EGSnrc-based BEAMnrc codes were used to generate the phase space files (SSD=100cm, FS=40×40cm2) for the linac (linear accelerator, Varian 21EX, 6MV photon mode) and EGSnrc-based DOSXYZnrc code was used to calculate the dose in the region of interest. Interpolation of depth dose curves of pre-set energies was proposed as a preliminary step for optimal energy fit. A good approach for determination of the optimal mean energy is the difference comparison of the PDD curves excluding buildup region, and using D(10) as a normalization method. For FWHM fitting, due to electron disequilibrium and the larger statistical uncertainty, using horn or/and penumbra regions will give inconsistent outcomes at various depths. Difference comparisons should be performed in the flat regions of the off-axis dose profiles at various depths to optimize the FWHM parameter. ► Crucial parameters were investigated using a logical system procedure. ► Interpolation of depth dose curves using pre-set energies as a first step. ► Comparisons using PDD curves normalized by D(10), excluding buildup region. ► FWHM is sensitive to horn/penumbra regions, but they give inconsistent values. ► Optimizing the FWHM requires the flat regions at various depths.
ISSN:0969-806X
1879-0895
DOI:10.1016/j.radphyschem.2013.02.017