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arXiv 2005.03061physics.ins-detcond-mat.otherhep-exnucl-exphysics.atom-ph
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电场对快电子产生的液氦闪烁的影响

Effect of an electric field on liquid helium scintillation produced by fast electrons

N. S. Phan, V. Cianciolo, S. M. Clayton, S. A. Currie, R. Dipert, T. M. Ito, S. W. T. MacDonald, C. M. O'Shaughnessy, J. C. Ramsey, G. M. Seidel, E. Smith, E. Tang, Z. Tang, W. Yao

AI总结:

本文研究电场对液氦中快电子和α粒子闪烁光的影响,发现温度依赖性源于双子对复合时间与信号积分时间的关系,并揭示次级电子空间分布的非高斯尾部,为粒子探测的脉冲形状分析提供新见解。

摘要:

本文报告了在0.44 K至3.12 K温度范围内,快电子和α粒子在液氦中停止时产生的闪烁光对外加电场(0-40 kV/cm)的依赖性。对于两种类型的粒子,由于外加电场导致的闪烁信号强度降低表现出明显的温度依赖性。利用德拜-斯莫卢霍夫斯基方程的近似解,我们表明电子的表观温度依赖性可以通过双子对复合所需时间相对于探测器信号积分时间的关系来解释。这一发现表明,次级电子相对于其双子伙伴的空间分布在大分离距离处具有重的非高斯尾部,并且依赖于初级电离电子的能量。我们讨论了这一结果在粒子探测和鉴别中脉冲形状分析方面的潜在应用。

英文摘要:

The dependence on applied electric field ($0 - 40$ kV/cm) of the scintillation light produced by fast electrons and $α$ particles stopped in liquid helium in the temperature range of 0.44 K to 3.12 K is reported. For both types of particles, the reduction in the intensity of the scintillation signal due to the applied field exhibits an apparent temperature dependence. Using an approximate solution of the Debye-Smoluchowski equation, we show that the apparent temperature dependence for electrons can be explained by the time required for geminate pairs to recombine relative to the detector signal integration time. This finding indicates that the spatial distribution of secondary electrons with respect to their geminate partners possesses a heavy, non-Gaussian tail at larger separations, and has a dependence on the energy of the primary ionization electron. We discuss the potential application of this result to pulse shape analysis for particle detection and discrimination.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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