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arXiv 1106.0167physics.ins-dethep-ex
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低温光探测器:Neganov-Luke放大和校准

Low-Temperature Light Detectors: Neganov-Luke Amplification and Calibration

C. Isaila, C. Ciemniak, F. v. Feilitzsch, A. Gütlein, J. Kemmer, T. Lachenmaier, J. -C. Lanfranchi, S. Pfister, W. Potzel, S. Roth, M. v. Sivers, R. Strauss, W. Westphal, F. Wiest

摘要:

同时测量声子和闪烁光的入射粒子在闪烁晶体,如CaWO 4是一个强大的技术,主动排斥的背景诱导的γ和β的,甚至中子在直接暗物质搜索。然而,在CaWO 4晶体中沉积的能量中,只有不到1%被检测为光。因此,需要非常灵敏的光检测器来进行有效的逐事件背景辨别。利用Neganov-Luke效应,通过在外加电场中漂移光生电子空穴对,可以显著提高基于半导体衬底的低温光探测器的阈值。我们目前的测量与低温光探测器的基础上,这种放大机制。Neganov-Luke效应使我们的光探测器的信噪比提高了约9倍,对应于约21 eV的能量阈值。我们还描述了一种使用发光二极管进行绝对能量校准的方法。

英文摘要:

The simultaneous measurement of phonons and scintillation light induced by incident particles in a scintillating crystal such as CaWO4 is a powerful technique for the active rejection of background induced by gamma's and beta's and even neutrons in direct Dark Matter searches. However, less than ~1% of the energy deposited in a CaWO4 crystal is detected as light. Thus, very sensitive light detectors are needed for an efficient event-by-event background discrimination. Due to the Neganov-Luke effect, the threshold of low-temperature light detectors based on semiconducting substrates can be improved significantly by drifting the photon-induced electron-hole pairs in an applied electric field. We present measurements with low-temperature light detectors based on this amplification mechanism. The Neganov-Luke effect makes it possible to improve the signal-to-noise ratio of our light detectors by a factor of ~9 corresponding to an energy threshold of ~21 eV. We also describe a method for an absolute energy calibration using a light-emitting diode.

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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