The use of deuteron microbeam for simulating the biological effects of heavy cosmic-ray particles.

H. Curtis
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引用次数: 84

Abstract

atomic nuclei of elements heavier than carbon and as heavy as iron. They are stripped of their electrons and thus are highly charged. As these particles are slowed down in tissue, they interact with the elements of the tissue and cause very energetic 6 rays to be emitted. The result is a track in tissue having very dense ionization near the end of its path, and this is known as a "thindown." This thindown region may be as much as 0.025 mm in diameter and 1.5 mm long. Schaefer (1) has computed that the radiation dose in this ionization core may be as much as 10,000 rads at its center, tapering off to low values toward the edges. Only the particles having energies less than about one billion electron volts per nucleon will cause this type of damage, since particles of higher energies will form stars and dissipate their energies widely. It would be virtually impossible to shield against these latter particles in a space craft because even a very heavy shield would only slow down the very energetic particles to the point where they would become highly ionizing and thus dangerous. In assessing the biological effect of such particles it would obviously not be correct to apply the usual rules for tolerance doses-that is, to compute the total dose from the energy deposited in the body of an average man. For heavy particles the energy is all deposited in very small volumes, or "hot spots," leaving the rest unaffected. This then constitutes a special radiobiological problem. These particles cannot presently be generated in the laboratory with sufficient energy to be used for mammalian experiments. Consequently an indirect experimental approach had to be developed (2). This consisted in confining the 22-MeV deuterons from the Brookhaven 60-inch cyclotron in a beam 0.025 mm in diameter. This microbeam was arranged in such a way that it could be directed at any pre1 Research carried out at Brookhaven National Laboratory under the auspices of the U. S.
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用氘核微束模拟重宇宙射线粒子的生物效应。
比碳重和铁重的元素的原子核。它们被剥夺了电子,因此带高电荷。当这些粒子在组织中减速时,它们会与组织中的元素相互作用,并发出非常有能量的射线。其结果是组织中的轨迹在其路径的末端具有非常密集的电离,这被称为“薄化”。这个薄化区域的直径可达0.025毫米,长1.5毫米。Schaefer(1)已经计算出这个电离核心的辐射剂量在其中心可能高达10,000拉德,在其边缘逐渐减少到低值。只有能量低于每核子10亿电子伏特的粒子才会造成这种类型的破坏,因为能量更高的粒子会形成恒星并广泛耗散它们的能量。要在宇宙飞船上屏蔽后一种粒子几乎是不可能的,因为即使是很重的屏蔽也只会使高能粒子减慢到高度电离的程度,从而产生危险。在评估这些粒子的生物效应时,应用通常的耐受剂量规则显然是不正确的,即计算普通人体内储存的能量的总剂量。对于重粒子,能量全部沉积在非常小的体积或“热点”中,其余部分不受影响。这就构成了一个特殊的放射生物学问题。这些粒子目前还不能在实验室中产生足够的能量用于哺乳动物实验。因此,必须开发一种间接实验方法(2)。这包括将来自布鲁克海文60英寸回旋加速器的22 mev氘核限制在直径0.025 mm的光束中。这束微光束被安排在这样一种方式,它可以被引导到任何在布鲁克海文国家实验室进行的研究。
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