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迈向基于桌面型飞秒硬X射线源的散粒噪声极限衍射实验。

Towards shot-noise limited diffraction experiments with table-top femtosecond hard x-ray sources.

作者信息

Holtz Marcel, Hauf Christoph, Weisshaupt Jannick, Salvador Antonio-Andres Hernandez, Woerner Michael, Elsaesser Thomas

机构信息

Max-Born-Institut für Nichtlineare Optik und Kurzzeitspektroskopie, 12489 Berlin, Germany.

出版信息

Struct Dyn. 2017 Jul 19;4(5):054304. doi: 10.1063/1.4991355. eCollection 2017 Sep.

DOI:10.1063/1.4991355
PMID:28795079
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5517321/
Abstract

Table-top laser-driven hard x-ray sources with kilohertz repetition rates are an attractive alternative to large-scale accelerator-based systems and have found widespread applications in x-ray studies of ultrafast structural dynamics. Hard x-ray pulses of 100 fs duration have been generated at the Cu K wavelength with a photon flux of up to 10 photons per pulse into the full solid angle, perfectly synchronized to the sub-100-fs optical pulses from the driving laser system. Based on spontaneous x-ray emission, such sources display a particular noise behavior which impacts the sensitivity of x-ray diffraction experiments. We present a detailed analysis of the photon statistics and temporal fluctuations of the x-ray flux, together with experimental strategies to optimize the sensitivity of optical pump/x-ray probe experiments. We demonstrate measurements close to the shot-noise limit of the x-ray source.

摘要

具有千赫兹重复率的桌面式激光驱动硬X射线源是基于大型加速器的系统的一种有吸引力的替代方案,并已在超快结构动力学的X射线研究中得到广泛应用。在Cu K波长处已产生持续时间为100 fs的硬X射线脉冲,每个脉冲进入全立体角的光子通量高达10个光子,与来自驱动激光系统的亚100 fs光脉冲完美同步。基于自发X射线发射,此类源表现出一种特殊的噪声行为,这会影响X射线衍射实验的灵敏度。我们对X射线通量的光子统计和时间涨落进行了详细分析,并提出了优化光泵浦/X射线探测实验灵敏度的实验策略。我们展示了接近X射线源散粒噪声极限的测量结果。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/559ccb02a746/SDTYAE-000004-054304_1-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/ce639fcca728/SDTYAE-000004-054304_1-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/a7d9a98d6266/SDTYAE-000004-054304_1-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/82adb3b41073/SDTYAE-000004-054304_1-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/f4313e19b47e/SDTYAE-000004-054304_1-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/d1a66fd36669/SDTYAE-000004-054304_1-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/9105457f65b6/SDTYAE-000004-054304_1-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/559ccb02a746/SDTYAE-000004-054304_1-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/ce639fcca728/SDTYAE-000004-054304_1-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/a7d9a98d6266/SDTYAE-000004-054304_1-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/82adb3b41073/SDTYAE-000004-054304_1-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/f4313e19b47e/SDTYAE-000004-054304_1-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/d1a66fd36669/SDTYAE-000004-054304_1-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/9105457f65b6/SDTYAE-000004-054304_1-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/17ca/5517321/559ccb02a746/SDTYAE-000004-054304_1-g007.jpg

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