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Diagnosing fuel rho R and rho R asymmetries in cryogenic deuterium-tritium implosions using charged-particle spectrometry at OMEGA

机译:使用OMEGA的带电粒子光谱技术诊断低温氘-tri内爆中的燃料rho R和rho R不对称性

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摘要

Determining fuel areal density (rho R) in moderate-rho R (100-200 mg/cm(2)) cryogenic deuterium-tritium (DT) implosions is challenging as it requires new spectrometry techniques and analysis methods to be developed. In this paper, we describe a new method for analyzing the spectrum of knock-on deuterons (KO-Ds), elastically scattered by primary DT neutrons, from which a fuel rho R can be inferred for values up to similar to 200 mg/cm(2). This new analysis method, which uses Monte Carlo modeling of a cryogenic DT implosion, improves significantly the previous analysis method in two fundamental ways. First, it is not affected by significant spatial-yield variations, which degrade the diagnosis of the fuel rho R (spatial yield variations of about +/- 20% are typically observed), and second, it does not break down when the fuel rho R exceeds similar to 70 mg/cm(2).
机译:确定中度R R(100-200 mg / cm(2))低温氘-tri(DT)内爆的燃料面密度(rho R)具有挑战性,因为它需要开发新的光谱技术和分析方法。在本文中,我们描述了一种新的方法,用于分析由主要DT中子弹性散射的连锁氘核(KO-Ds)的光谱,由此可以推断出燃料Rho R的值高达200 mg / cm (2)。这种新的分析方法使用了低温DT内爆的蒙特卡洛模型,在两个基本方面显着改进了先前的分析方法。首先,它不受显着的空间-产量变化的影响,这会降低燃料rho R的诊断能力(通常会观察到大约+/- 20%的空间产量变化),其次,当燃料rho R下降时,它不会分解R超过类似于70 mg / cm(2)。

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