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作为高能量密度科学中X射线源的动态黑腔

Dynamic Hohlraums as x-ray sources in high-energy density science.

作者信息

Hansen J F, Glendinning S G, Heeter R F, Brockington S J E

机构信息

Lawrence Livermore National Laboratory, Livermore, California 94550, USA.

出版信息

Rev Sci Instrum. 2008 Jan;79(1):013504. doi: 10.1063/1.2804765.

Abstract

The first demonstration of laser driven dynamic Hohlraums (LDDH) as a spectrally smooth backlighter source for opacity and temperature measurements through absorption spectrometry of materials in local thermodynamic equilibrium at temperatures >150 eV has been made. This is a crucial temperature regime for future astrophysics and ignition fusion experiments at the nearly completed National Ignition Facility (NIF) [E. I. Moses and C. R. Wuest, Fusion Sci. Technol. 47, 314 (2005)] at the Lawrence Livermore National Laboratory. The new backlighter consists of a LDDH filled with either krypton or argon that implodes to create an x-ray flash. The properties of this x-ray flash have been measured in experiments at the Omega laser [T. R. Boehly et al., Opt. Commun. 133, 495 (1997)] at the Laboratory for Laser Energetics in Rochester, New York, satisfying all requirements imposed by future experiments: (1) the emission spectrum extends to at least 5.5 keV, well above the maximum x-ray energy ( approximately 3.5 keV) obtained from the previously "best" opacity backlighters (uranium M-shell emission backlighters); (2) the spectrum is smooth and featureless (intensity variation <6% rms), allowing absorption spectrometry through experimental samples; (3) the emission source size is sufficiently small (<50 microm) for projection backlighting through future samples; (4) the emission is bright enough (and twice as bright as imploding hydrogen-filled capsules) for gated spectrometer measurements; (5) the emission duration is optimized ( approximately 100 ps) for the current and future generations of spectrometers; and (6) by using only a small number of beams with limited energy and symmetry for the backlighter (10 out of 60 beams in the Omega experiments), the majority of laser beams are left available for heating sample materials to >150 eV.

摘要

首次证明了激光驱动动态黑腔(LDDH)可作为一种光谱平滑的背光源,用于通过对处于温度>150eV的局部热力学平衡状态下的材料进行吸收光谱法来测量不透明度和温度。对于未来的天体物理学以及劳伦斯利弗莫尔国家实验室几乎建成的国家点火装置(NIF)[E. I. 摩西和C. R. 韦斯特,《聚变科学与技术》47, 314 (2005)]上的点火聚变实验而言,这是一个关键的温度范围。这种新型背光源由充满氪或氩的LDDH组成,其向内爆聚以产生X射线闪光。该X射线闪光的特性已在纽约罗切斯特激光能量学实验室的欧米茄激光器[T. R. 博埃利等人,《光学通信》133, 495 (1997)]上进行的实验中测量,满足了未来实验提出的所有要求:(1)发射光谱至少延伸至5.5keV,远高于从先前“最佳”不透明度背光源(铀M壳层发射背光源)获得的最大X射线能量(约3.5keV);(2)光谱平滑且无特征(强度变化<6%均方根误差),允许通过实验样品进行吸收光谱法测量;(3)发射源尺寸足够小(<50微米),可用于对未来样品进行投影背光照相;(4)发射亮度足够高(是向内爆聚的充氢胶囊亮度的两倍),可用于门控光谱仪测量;(5)发射持续时间针对当前及下一代光谱仪进行了优化(约100皮秒);(6)通过仅使用少量能量和对称性有限的光束作为背光源(欧米茄实验中60束光束中的10束),大部分激光束可留作加热样品材料至>150eV之用。

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