Plante Ianik, Ponomarev Artem, Cucinotta Francis A
NASA Johnson Space Center, 2101 NASA Parkway, Houston, TX 77058, USA.
Radiat Prot Dosimetry. 2011 Feb;143(2-4):156-61. doi: 10.1093/rpd/ncq526. Epub 2011 Jan 2.
The description of energy deposition by high charge and energy (HZE) nuclei is of importance for space radiation risk assessment and due to their use in hadrontherapy. Such ions deposit a large fraction of their energy within the so-called core of the track and a smaller proportion in the penumbra (or track periphery). We study the stochastic patterns of the radial dependence of energy deposition using Monte Carlo track structure codes RITRACKS and RETRACKS, that were used to simulate HZE tracks and calculate energy deposition in voxels of 40 nm. The simulation of a (56)Fe(26+) ion of 1 GeV u(-1) revealed zones of high-energy deposition which maybe found as far as a few millimetres away from the track core in some simulations. The calculation also showed that ∼43 % of the energy was deposited in the penumbra. These 3D stochastic simulations combined with a visualisation interface are a powerful tool for biophysicists which may be used to study radiation-induced biological effects such as double strand breaks and oxidative damage and the subsequent cellular and tissue damage processing and signalling.
高电荷和能量(HZE)核的能量沉积描述对于太空辐射风险评估以及在强子治疗中的应用都很重要。这类离子将其大部分能量沉积在所谓的径迹核心内,而在半影区(或径迹周边)沉积的比例较小。我们使用蒙特卡罗径迹结构代码RITRACKS和RETRACKS研究能量沉积径向依赖性的随机模式,这些代码用于模拟HZE径迹并计算40纳米体素中的能量沉积。对能量为1 GeV u(-1)的(56)Fe(26+)离子的模拟揭示了高能沉积区域,在某些模拟中,这些区域可能在距离径迹核心几毫米远的地方被发现。计算还表明,约43%的能量沉积在半影区。这些三维随机模拟与可视化界面相结合,对于生物物理学家来说是一个强大的工具,可用于研究辐射诱导的生物效应,如双链断裂和氧化损伤,以及随后的细胞和组织损伤处理与信号传导。