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Time-Frequency Analysis of Asymmetric Triaxial Galaxy Model Including Effect of Spherical Dark Halo Component

机译:含球形暗晕分量影响的非对称三轴星系模型时频分析

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A method of time-frequency analysis (TFA) based on wavelets is applied to study the phase space structure of three-dimensional asymmetric triaxial galaxy enclosed by spherical dark halo component. The investigation is carried out in the presence and absence of dark halo component. Time-frequency analysis is based on the extraction of instantaneous frequency from the phase of the continuous wavelet transform. This method is comparatively fast and reliable. This method can differentiate periodic from quasi-periodic, chaotic sticky from chaotic non-sticky, ordered from chaotic and also, it can accurately determine the time interval of the resonance trapping and transitions too. Apart from that, the phenomenon of transient chaos can be explained with the help of time-frequency analysis. Comparison with the method of total angular momentum (denoted as Ltot) proposed recently is also presented.
机译:提出了一种基于小波的时频分析方法,研究了球形暗晕分量包围的三维非对称三轴星系的相空间结构。在存在和不存在暗晕成分的情况下进行研究。时频分析基于从连续小波变换的相位中提取瞬时频率。这种方法比较快速可靠。该方法可以区分周期性与准周期性,混沌粘性与混沌非粘性,混沌有序性,还可以准确地确定共振陷获和跃迁的时间间隔。除此之外,可以通过时频分析来解释瞬态混沌现象。还提出了与最近提出的总角动量方法(称为Ltot)的比较。

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