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利用 X 射线自由电子激光产生和诊断固体密度等离子体。

Creation and diagnosis of a solid-density plasma with an X-ray free-electron laser.

机构信息

Department of Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford OX1 3PU, UK.

出版信息

Nature. 2012 Jan 25;482(7383):59-62. doi: 10.1038/nature10746.

Abstract

Matter with a high energy density (>10(5) joules per cm(3)) is prevalent throughout the Universe, being present in all types of stars and towards the centre of the giant planets; it is also relevant for inertial confinement fusion. Its thermodynamic and transport properties are challenging to measure, requiring the creation of sufficiently long-lived samples at homogeneous temperatures and densities. With the advent of the Linac Coherent Light Source (LCLS) X-ray laser, high-intensity radiation (>10(17) watts per cm(2), previously the domain of optical lasers) can be produced at X-ray wavelengths. The interaction of single atoms with such intense X-rays has recently been investigated. An understanding of the contrasting case of intense X-ray interaction with dense systems is important from a fundamental viewpoint and for applications. Here we report the experimental creation of a solid-density plasma at temperatures in excess of 10(6) kelvin on inertial-confinement timescales using an X-ray free-electron laser. We discuss the pertinent physics of the intense X-ray-matter interactions, and illustrate the importance of electron-ion collisions. Detailed simulations of the interaction process conducted with a radiative-collisional code show good qualitative agreement with the experimental results. We obtain insights into the evolution of the charge state distribution of the system, the electron density and temperature, and the timescales of collisional processes. Our results should inform future high-intensity X-ray experiments involving dense samples, such as X-ray diffractive imaging of biological systems, material science investigations, and the study of matter in extreme conditions.

摘要

高能量密度物质(>10(5)焦耳每立方厘米)在整个宇宙中都很普遍,存在于所有类型的恒星和巨行星的中心;它也与惯性约束聚变有关。其热力学和输运性质难以测量,需要在均匀温度和密度下创建足够长寿命的样品。随着直线感应加速器相干光源(LCLS)X 射线激光的出现,高强度辐射(>10(17)瓦特每平方厘米,以前是光学激光的领域)可以在 X 射线波长下产生。最近,人们研究了单个原子与如此高强度 X 射线的相互作用。从基础观点和应用角度来看,了解密集系统与高强度 X 射线相互作用的对比情况非常重要。在这里,我们使用 X 射线自由电子激光在惯性约束时间尺度上报告了在超过 10(6)开尔文温度下的固体密度等离子体的实验创建。我们讨论了高强度 X 射线与物质相互作用的相关物理问题,并说明了电子-离子碰撞的重要性。使用辐射-碰撞代码进行的相互作用过程的详细模拟与实验结果具有良好的定性一致性。我们深入了解了系统电荷状态分布、电子密度和温度以及碰撞过程时间尺度的演化。我们的结果应该为未来涉及密集样品的高强度 X 射线实验提供信息,例如生物系统的 X 射线衍射成像、材料科学研究以及极端条件下物质的研究。

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