Omar Artur, Andreo Pedro, Poludniowski Gavin
Medical Radiation Physics and Nuclear Medicine, Karolinska University Hospital, Stockholm, 17176, Sweden.
Department of Oncology-Pathology, Karolinska Institutet, Stockholm, 17176, Sweden.
Med Phys. 2020 Sep;47(9):4005-4019. doi: 10.1002/mp.14360. Epub 2020 Jul 18.
To present and validate a complete x-ray emission model (bremsstrahlung and characteristic x-ray emission) for the energy range 20-300 kV.
An analytical x-ray spectrum model that combines the bremsstrahlung emission model developed in Part I with a previously developed characteristic x-ray emission model is validated by comparison with Monte Carlo calculations, published measured spectra, and models developed by other authors. Furthermore, the assumptions and limitations of previous spectrum models are summarized, and their predictions are compared with results obtained by Monte Carlo simulations of x rays emitted from tungsten and molybdenum targets.
The model is able to reproduce narrow-beam Monte Carlo calculations to within 0.5% in terms of the first and second aluminum half-value layer thickness (HVL). Compared with measured spectra, the difference in HVL is < 2% for typical diagnostic and therapeutic beam qualities available at primary standard laboratories. Compared with previous spectrum models, the present model performs especially well for low kilovoltage x-ray beams (below 50 kV), and is reliable for a wider range of take-off angles, that is, the angle between the target surface and the direction of emission. The difference in model and Monte Carlo predictions of the energy-fluence weighted air kerma (i.e., the photon energy absorption in air) is < 0.5% using the present model, while previous spectrum models can differ by more than 10%.
The x-ray emission model developed in this work has been validated against Monte Carlo calculations and measured results. The model provides an efficient alternative to comprehensive Monte Carlo simulations and is an improvement over previous models. The model can be used to predict both central- and off-axis spectra, as well as off-axis effects such as the (anode) heel effect.
提出并验证一个适用于20 - 300 kV能量范围的完整X射线发射模型(轫致辐射和特征X射线发射)。
通过与蒙特卡罗计算、已发表的测量光谱以及其他作者开发的模型进行比较,验证了一个将第一部分中开发的轫致辐射发射模型与先前开发的特征X射线发射模型相结合的分析X射线光谱模型。此外,总结了先前光谱模型的假设和局限性,并将它们的预测结果与通过对钨和钼靶发射的X射线进行蒙特卡罗模拟得到的结果进行比较。
就第一和第二铝半值层厚度(HVL)而言,该模型能够将窄束蒙特卡罗计算结果重现至0.5%以内。与测量光谱相比,对于初级标准实验室中可用的典型诊断和治疗束质,HVL的差异小于2%。与先前的光谱模型相比,本模型在低千伏X射线束(低于50 kV)方面表现尤其出色,并且对于更广泛的出射角范围(即靶表面与发射方向之间的角度)是可靠的。使用本模型时,模型与蒙特卡罗对能量通量加权空气比释动能(即空气中的光子能量吸收)的预测差异小于0.5%,而先前的光谱模型差异可能超过10%。
本工作中开发的X射线发射模型已通过与蒙特卡罗计算和测量结果进行验证。该模型为全面的蒙特卡罗模拟提供了一种有效的替代方法,并且是对先前模型的改进。该模型可用于预测中心轴和离轴光谱,以及离轴效应,如(阳极)足跟效应。