减少掺杂剂直接驱动预热

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS High Energy Density Physics Pub Date : 2021-06-01 DOI:10.1016/j.hedp.2021.100937
T.R. Desjardins, C.A. Di Stefano, E.C. Merritt, K.A. Flippo, F.W. Doss
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引用次数: 3

摘要

激光驱动实验中的预热会对惯性约束聚变(ICF)和流体动力实验产生负面影响。虽然许多小组使用掺杂剂来减少或阻止预热,但以前没有探索过直接量化。我们开发了一个平面平台和一系列烧蚀靶,以测量由OMEGA-60直接驱动的激光等离子体相互作用产生的电子和x射线光谱。通过比较纯CH、掺3% Si或掺3% I的薄烧蚀体(75米)和厚烧蚀体(270米),我们能够测量电子和x射线光谱的差异。此外,我们观察到示踪层的预热生长,并观察到不同材料的示踪层的生长减少。我们发现碘或薄金层在OMEGA直接驱动预热时的夯实效果最好,但其增长仍然显著。
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Reducing direct drive preheat with dopants

Preheat in laser-driven experiments can have negative impacts on inertial confinement fusion (ICF) and hydrodynamic experiments. While many groups employ the use of dopants to reduce or block preheat, direct quantification has not previously been explored. We developed a planar platform and a series of ablator targets to measure the electron and x-ray spectra generated by laser-plasma interactions with a direct drive using OMEGA-60. By comparing both thin ablators (75m) and thick ablators (270 m) that were either pure CH, 3% Si doped or 3% I doped, we were able to measure differences in electron and x-ray spectra. In addition, we observed the preheat growth of tracer layers and observed reductions in the growth with different materials. We find that iodine or a thin gold layer is the best at tamping the direct-drive preheat at OMEGA, but that the growth is still significant.

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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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