模拟DNA链断裂实验的核小体模型。

M Terrissol, E Pomplun
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引用次数: 8

摘要

利用蒙特卡罗模拟模型,将液态水中产生的125I俄热电子的轨道结构叠加到核小体DNA模型上,该模型能够精确定位DNA链亚分子单元上的能量沉积事件。在物理阶段(大约10(-15)秒)进行直接命中后,在10(-12)到10(-8)秒之间模拟整个系统的辐射化学,考虑到水中放射性化学物质、自由基、DNA亚分子单位(核糖、腺嘌呤、胸腺嘧啶、鸟嘌呤和胞嘧啶)以及Tris或甲酸离子等清除剂之间的所有反应。利用该模型区分直接和间接撞击的可能性,引入了两种撞击模式诱导链断裂的不同假设。将给出SSB和DSB的数量及其局部分布,并与文献中的实验和理论结果进行比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A nucleosome model for the simulation of DNA strand break experiments.

Using a set of Monte Carlo simulation models, track structures of 125I Auger electrons generated in liquid water are superimposed on a nucleosome DNA model able to precisely localize energy deposition events on sub-molecular units of the DNA strands. After scoring direct hits taking place during the physical phase (at about 10(-15) s) the radiation chemistry of the whole system is simulated between 10(-12) and 10(-8) s, taking into account all reactions between water radio-chemical species, radicals, sub-molecular units of DNA (Ribose, Adenine, Thymine, Guanine, and Cytosine), and scavengers like Tris or Formate ions. The model's possibility to distinguish between direct and indirect hits has been utilized to introduce different assumptions for strand break induction by both hit modes. The number of SSB and DSB as well as their local distribution will be given and compared with experimental and theoretical results from the literature.

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