MECHANISM OF SCINTILLATION OF HELIUM, HELIUM--ARGON, AND HELIUM--NEON GAS MIXTURES EXCITED BY ALPHA PARTICLES.
MECHANISM OF SCINTILLATION OF HELIUM, HELIUM--ARGON, AND HELIUM--NEON GAS MIXTURES EXCITED BY ALPHA PARTICLES.
复制标题
由 α 粒子激发的氦、氦-氩和氦-氖气体混合物的闪烁机制。
DOI:
10.1103/physrev.165.225
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发表时间:
1968
期刊:
影响因子:
--
通讯作者:
T. Doke
中科院分区:
文献类型:
--
作者:
S. Kubota;T. Takahashi;T. Doke
An experimental investigation of the mechanism of scintillation of helium, helium-argon, and helium-neon mixtures excited by α particles has been performed. No detectable decrease in light yield was observed at pressures less than 3 atm when the applied electric field was increased in steps to E p∼ 1.0 V/cm Torr, where E is the electric field and p is the gas pressure. The pulse shape of helium scintillation light consists of a slow component and a spike appearing on the leading edge of the pulse. The main component of light intensity is represented by the formula exp (− t τ m)− exp (− t τ f), where t is the time in sec, τ m= 10× 10− 6 sec, and τ f= 0.3 p− 2.2±0.3 sec (p in Torr). Most of the emitted photons had a wavelength of less than 1050 ÅA. On the basis of these results, it is concluded that the emitted photons are released in the decay of excited helium molecules formed as a result of a three-body collision between a metastable and two ground-state helium atoms. A characteristic large drop in the light yield for a mixture of a small proportion of argon in a major fraction of helium can be explained by the production of argon ions by metastable helium atoms (Penning process). The same characteristic large drop for a mixture of small concentration of neon in helium seems to be caused by the excitation transfer from helium to neon atoms. The cross section σ f for the formation of an excited helium molecule by a three-body collision is estimated to be 50× 10− 23 p cm 2 at 300 K, where p is in Torr. From the value of σ f, the cross section σ i of the helium-argon Penning process is calculated as 41× 10− 16 and 14× 10− 16 cm 2 by using the ratios of σ i to σ f estimated by Jesse and Sadauskis and by Northrop and Gursky, respectively.