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Processes driving non-Maxwellian distributions in high energy density plasmas

机译:在高能量密度等离子体中驱动非麦克斯韦分布的过程

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摘要

The purpose of this thesis is to explore the driving of non-Maxwellian distributions of particles in high energy density plasmas in a few select cases, with particular reference to efforts to produce a net gain in energy via inertial confinement fusion (ICF). ududNon-Maxwellian distributions are typically short-lived, as distributions are forced toward equilibrium by collisions, and are rarely static as a net transfer of energy must occur to sustain them. This makes non-Maxwellian distributions challenging to study with conventional approaches to plasma physics. The strategy adopted in this work to understand their evolution, and their effects, is a kinetic approach in which particles are individually accounted for.ududThe specific cases presented are that of degenerate electrons during the heating of the cold fuel shell in hotspot ignition schemes, ion-ion inverse bremsstrahlung absorption of laser radiation, and large-angle Coulomb collisions. New computational algorithms based on the Monte Carlo technique are presented, and are capable of modelling the salient aspects of the phenomena explored. Important results which form part of this thesis include that conventional models underestimate degenerate electron temperatures long after the plasma ceases to be degenerate, that it may be possible to induce temperatures of keV in light-ion species with high power, short pulse lasers, and that consideration of large-angle collisions changes interactions in a plasma in several significant ways. Of most interest are the ability of large-angle collisions to decrease equilibration times, drive athermal tails on distribution functions, and increase the overall yield from fusion reactions relative to small-angle only simulations.
机译:本文的目的是探索在某些特定情况下高能密度等离子体中非马克斯韦尔粒子分布的驱动,特别是通过惯性约束聚变(ICF)产生能量净收益的努力。非Maxwellian分布通常是短暂的,因为碰撞会迫使这些分布趋于平衡,并且由于必须发生能量的净传递才能维持它们的分布,因此很少是静态的。这使得非麦克斯韦分布很难用等离子体物理的常规方法进行研究。在这项工作中采用的了解其演化及其作用的策略是一种动力学方法,其中单独考虑了颗粒。 ud ud所呈现的特定情况是在热点点火中冷燃料壳加热期间简并电子的情况。方案,激光辐射的离子反致辐射吸收和大角度库仑碰撞。提出了基于蒙特卡洛技术的新计算算法,并且能够对所探究现象的显着方面进行建模。构成本论文一部分的重要结果包括:常规模型低估了等离子体停止退化后很长时间内退化的电子温度;使用高功率,短脉冲激光,有可能在轻离子物种中诱发keV温度。考虑大角度碰撞会以几种重要方式改变等离子体中的相互作用。相对于仅使用小角度的模拟,最感兴趣的是大角度碰撞减少平衡时间,在分布函数上驱动无热尾部并提高融合反应的总产率的能力。

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    Turrell Arthur Edward;

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