间接驱动产量灵敏度厚壳模型

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
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引用次数: 0

摘要

我们提出了间接驱动 ICF 内爆的解析厚壳模型,首先使用火箭方程评估燃料动能峰值,然后通过能量平衡评估停滞燃料内能。然后,我们使用热点绝热减速到等压停滞状态的近似方法,并结合自洽计算的燃料长宽比。该模型经过一维辐射流体力学模拟验证,提供了间接驱动产率、DSR 和点火指标对一系列初始和最终状态胶囊和霍尔姆参数的敏感性,适用于当前相关的点火内爆机制。该模型用于强调参数权衡,并估算在当前和更高的性能水平下,一维压缩、停滞面积密度和当量的预期灵敏度。我们提出了一些新的见解。值得注意的是,我们解释了具有埋藏掺杂层设计的消融器厚度对内爆速度的微弱依赖性、添加燃料或降低初始热点密度时性能改进的不确定性,以及电离能和反照率在设定消融器效率中的作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thick-shell model of indirect-drive yield sensitivity

We present an analytic thick shell model for indirect-drive ICF implosions that starts by using the Rocket equation to evaluate peak fuel kinetic energy and hence by energy balance, stagnated fuel internal energy. We then use the approximation of the hot spot decelerating adiabatically to an isobaric stagnated state coupled to a self-consistently calculated fuel aspect ratio. The model, validated by 1D radiation-hydrodynamics simulations, provides sensitivities of indirect-drive yield, DSR and ignition metrics to a host of initial and final state capsule and hohlraum parameters, applicable to the current relevant regime of igniting implosions. The model is used to highlight parameter trade-offs and estimate expected sensitivity in 1D compression, stagnated areal density and yield at current and higher performance levels. Several new insights are presented. Of note, we explain the weak dependence of ablator thickness on implosion velocity for designs with buried dopant layers, the uncertainty in performance improvement when adding fuel or reducing initial hot spot density, and the role of ionization energy and albedo in setting ablator efficiency.

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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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