论文标题

$^{210} $ pb在NAI(TL)水晶表面的深度概况研究

Depth profile study of $^{210}$Pb in the surface of an NaI(Tl) crystal

论文作者

Yu, G. H., Ha, C., Jeon, E. J., Kim, K. W., Kim, N. Y., Kim, Y. D., Lee, H. S., Park, H. K., Rott, C.

论文摘要

表面$^{210} $ pb是使用NAI(TL)晶体进行深色搜索实验的主要背景来源之一,其光谱特征与beta-decay事件相关的beta-decay事件小于60 keV取决于$^{210} $ pb的深度分布在NAI(TL)水晶的表面中。因此,我们必须了解使用NAI(TL)晶体的低能地面实验的低能区域中的表面$^{210} $ Pb的曲线。我们通过建模$^{210} $ po的α衰减,以表面$^{210} $ pb污染的衰减顺序对α排放的测量光谱进行建模,从而估计表面$^{210} $ pb污染的深度曲线。为了描述表面污染的能量光谱,我们对测量数据的对数似然拟合到Geant4 Mote Carlo模拟的总和,并由指数曲线加权,这是表面深度的函数。还对表面$^{210} $ PB的β衰减中的低能和高能事件进行了建模,以改善浅深度的深度曲线。我们通过遵循两个指数函数在表面上呈指数分布的$^{210} $ pb的β衰减的能量光谱,其中均值深度系数是数据拟合中的免费参数;我们观察到能量光谱与测量数据非常吻合。

The surface $^{210}$Pb is one of the main background sources for dark-matter-search experiments using NaI(Tl) crystals, and its spectral features associated with the beta-decay events for energies less than 60 keV depends on the depth distribution of $^{210}$Pb in the surface of an NaI(Tl) crystal. Therefore, we must understand the profile of surface $^{210}$Pb to precisely model the background measurement in the low-energy region for the low-background experiment using NaI(Tl) crystals. We estimate the depth profile of the surface $^{210}$Pb contamination by modeling the measured spectrum of the alpha emission from the decay of $^{210}$Po at the decay sequence of the surface $^{210}$Pb contamination that is obtained using an $^{222}$Rn-contaminated crystal. In order to describe the energy spectra of the surface contamination we perform a log-likelihood fit of the measured data to a sum of Geant4 Mote Carlo simulations, weighted by an exponential curve as a function of the surface depth. The low- and high-energy events from the beta decay of surface $^{210}$Pb are also modeled to improve the depth profile for shallow depths. We simulate the energy spectra from beta decays of $^{210}$Pb that are exponentially distributed in the surface by following two exponential functions where the mean-depth coefficients are free parameters in the data fitting; we observed that the energy spectra are in good agreement with the measured data.

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