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首页> 外文期刊>Nuclear Instruments & Methods in Physics Research >The threshold of gamma-ray induced bubble nucleation in superheated emulsion
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The threshold of gamma-ray induced bubble nucleation in superheated emulsion

机译:过热乳液中γ射线诱导泡沫成核的阈值

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The bubble nucleation in superheated emulsion starts with the formation of critical sized vapour embryo in the liquid. The homogeneous nucleation can be triggered due to the energy deposition by the different kinds of radiations. At lower degree of superheat, higher ionizing particles can trigger the bubble formation. As the degree of superheat increases, lower ionizing particles also become responsible for bubble nucleation. In the present work, the bubble nucleation by the lower ionizing particles, e.g. gamma-rays has been discussed. Experiments were performed with R-134a (C2H2F4, b.p. -26.3 degrees C) superheated droplets in presence of Cs-137 (662 keV, 5 mCi) gamma source. From the GEANT4.10.02 simulation, it is observed that near the threshold temperature of gamma-ray, stopping power of electron having energy corresponding to its highest value at the end of the track is mostly responsible for initiating a bubble nucleation, whereas with increase in temperature of the liquid, electrons of other energies could play role in the bubble nucleation process. The nucleation occurs due to the energy deposition by the produced electrons (secondary and higher order) at the end of their tracks within the liquid.
机译:过热乳液中的气泡成核以液体中的临界尺寸蒸汽胚胎的形成开始。通过不同种类的辐射能量沉积,可以引发均匀成核。在过热程度较低,更高的电离颗粒可以引发气泡形成。随着过热程度的增加,降低电离颗粒也负责泡沫成核。在本作工作中,泡沫含量通过较低的电离颗粒成核,例如,已经讨论了伽马射线。在CS-137(662keV,5MCI)γ源存在下,用R-134A(C 2 H 2 F 4,B.P.P.P.P.P.P.2C)过热液滴进行实验。从GEANT4.10.02仿真中,观察到,靠近伽马射线的阈值温度,轨道结束时具有对应于其最高值的电能的电力主要负责启动气泡成核,而随着增加的液体的温度,其他能量的电子可以在泡沫成核过程中发挥作用。由于在液体内的轨道的轨道结束时由所产生的电子(次级和高阶)的能量沉积而发生成核。

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