首页> 外文期刊>Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment >Development of 2 cm-square Hamamatsu avalanche photodiodes for high-resolution X-rays and γ-rays detection
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Development of 2 cm-square Hamamatsu avalanche photodiodes for high-resolution X-rays and γ-rays detection

机译:研发2平方厘米的滨松雪崩光电二极管,用于高分辨率X射线和γ射线检测

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The avalanche photodiodes (APDs) have attracted considerable attention in various field of experimental physics, but their uses are still limited in only a few experiments, possibly due to their small surface areas. Here, we report the development of the large-area (~20 mm square) APDs, for future applications to high-resolution X-rays and γ-rays detection. We have made two prototypes of reverse-type APDs based on different concepts, one consists of a 2 x 2 array of 10 x 10 mm~2 pixels (APD1) and the other is a monolithic pixel of 19 x 19 mm~2 size (APD2) to achieve a large effective area. By comparing the dark current and gain characteristics at room temperature (+20℃) and lightly cooled environment (-20℃), we quantitatively discussed the origin of predominant noise source at different temperatures. As a performance demonstration of newly developed APDs, we made a scintillation γ-ray detector consisting of a 20 x 20 x 5 mm~3 CsI(Tl) crystal and a 2 cm-square APD. The best FWHM energy resolution of 5.5±0.2% were obtained for 662 keV γ-rays at room temperature. Similarly, the best FWHM energy resolution of 8.5 ± 0.2% were obtained for 122 keV γ-rays at lightly cooled environment. We showed that the minimum detectable energy for scintillation light was 15keV at 20℃ and less than 5keV at - 20℃.
机译:雪崩光电二极管(APD)在实验物理的各个领域中引起了相当大的关注,但由于其表面积较小,它们的使用仍仅在少数几个实验中受到限制。在这里,我们报告了大面积(约20毫米见方)APD的发展,以供将来用于高分辨率X射线和γ射线检测。我们根据不同的概念制作了两个反向型APD原型,一个原型由2 x 2的10 x 10 mm〜2像素(APD1)阵列组成,另一个是19 x 19 mm〜2大小的单片像素( APD2)实现大的有效面积。通过比较室温(+ 20℃)和弱冷环境(-20℃)下的暗电流和增益特性,我们定量讨论了不同温度下主要噪声源的起源。作为新开发的APD的性能演示,我们制作了由20 x 20 x 5 mm〜3 CsI(Tl)晶体和2 cm见方的APD组成的闪烁γ射线探测器。室温下662 keVγ射线获得的最佳FWHM能量分辨率为5.5±0.2%。类似地,在轻度冷却的环境下,对于122 keVγ射线,最佳的FWHM能量分辨率为8.5±0.2%。我们表明,闪烁光的最小可探测能量在20℃为15keV,在-20℃小于5keV。

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