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Zinc Oxide Nanowire Gamma Ray Detector with High Spatiotemporal Resolution

机译:时空分辨率高的氧化锌纳米线伽马射线探测器

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Conventional scintillation detectors are typically single crystals of heavy-metal oxides or halides doped with rare-earth ions that record the recombination of electron-hole pairs by photon emission in the visible to ultraviolet. However, the light yields are typically low enough to require photomultiplier detection with the attendant instrumental complications. Here we report initial studies of gamma ray detection by zinc oxide (ZnO) nanowires, grown by vapor-solid deposition. The nanowires grow along the c-axis in a wurtzite structure; they are typically 80 nm in diameter and have lengths of 1-2 urn. The nanowires are single crystals of high quality, with a photoluminescence (PL) yield from band-edge exciton emission in the ultraviolet that is typically one hundred times larger than the PL yield from defect centers in the visible. Nanowire ensembles were irradiated by 662 keV gamma rays from a Cs-137 source for periods of up to ten hours; gamma rays in this energy range interact by Compton scattering, which in ZnO creates F~+ centers that relax to form singly-charged positive oxygen vacancies. Following irradiation, we fit the PL spectra of the visible emission with a sum of Gaussians at the energies of the known defects. We find highly efficient PL from the irradiated area, with a figure of merit approaching 10~6 photons/s/MeV of deposited energy. Over a period of days, the singly charged O~+ vacancies relax to the more stable doubly charged O~(++) vacancies. However, the overall defect PL returns to pre-irradiation values after about a week, as the vacancies diffuse to the surface of these very thin nanowires, indicating that a self-healing process restores the nanowires to their original state.
机译:常规的闪烁检测器通常是掺杂有稀土离子的重金属氧化物或卤化物的单晶,其通过可见光到紫外光中的光子发射来记录电子-空穴对的重组。但是,光输出通常足够低,以至于需要进行光电倍增管检测以及伴随的仪器并发症。在这里,我们报告了通过气相沉积法生长的氧化锌(ZnO)纳米线对伽马射线探测的初步研究。纳米线以纤锌矿结构沿c轴生长;它们的直径通常为80 nm,长度为1-2 um。纳米线是高质量的单晶,紫外线中带边激子发射的光致发光(PL)产量通常比可见缺陷中心的PL产量大一百倍。用来自Cs-137的662 keVγ射线辐照纳米线集合体长达10个小时。在此能量范围内的伽马射线通过康普顿散射相互作用,这在ZnO中产生F〜+中心,这些中心放松形成单电荷的正氧空位。辐照后,我们将可见光的PL光谱与已知缺陷能量下的高斯之和进行拟合。我们从辐照区域发现了高效的PL,其品质因数接近10〜6光子/ s / MeV的沉积能量。在几天的时间里,单电荷的O〜+空位放松到更稳定的双电荷的O〜(++)空位。然而,由于空位扩散到这些非常细的纳米线的表面,整个缺陷PL大约在一周后恢复到辐照前的值,这表明自我修复过程将纳米线恢复到其原始状态。

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