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Quantum chaos analysis of the ideal interchange spectrum in a stellarator

机译:恒星器中理想交换光谱的量子混沌分析

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The eigenmode spectrum is a fundamental starting point for the analysis of plasma stability and the onset of turbulence. Quantum chaos theory provides tools for characterizing the spectrum statistically, from the regular spectrum of the separable case (integrable semiclassical dynamics) to that where the semiclassical ray dynamics is so chaotic that no simple classification of the individual eigenvalues is possible (quantum chaos). Using the CAS3D code, a data set of several hundred growth-rate eigenvalues has been calculated for a Mercier-unstable three-dimensional stellarator equilibrium with a rather flat, non-monotonic rotational transform profile. Statistical analysis of eigenvalue spacings for individual mode families shows evidence of quantum chaos, strongest for the N = 0 family, but to test this we compare it with the distribution of eigenvalue spacings in a similar separable case-ideal interchange modes in a Suydam-unstable plasma cylinder-using, a similar rotational transform profile to the stellarator case. The statistics in the cylindrical model appear Poissonian, as expected for generic integrable systems and in clear contrast to the three-dimensional stellarator results.
机译:本征模谱是分析等离子体稳定性和湍流开始的基本起点。量子混沌理论提供了用于统计表征光谱的工具,从可分离情况的规则光谱(可积分的半经典动力学)到半经典射线动力学如此混乱以至于无法对单个特征值进行简单分类的量子混乱(量子混沌)。使用CAS3D代码,已经为具有相当平坦的非单调旋转变换轮廓的Mercier不稳定三维立体恒星计算了几百个增长率特征值的数据集。对各个模态族的特征值间隔的统计分析显示了量子混沌的证据,对于N = 0族来说最强,但是为了测试这一点,我们将其与在Suydam不稳定的类似可分离的案例-理想互换模式中的特征值间隔的分布进行了比较。等离子圆柱体的使用,类似于恒星箱的旋转变换轮廓。圆柱模型中的统计数据显示为泊松(Poissonian),这是一般可积系统所期望的,并且与三维恒星器结果形成鲜明对比。

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