论文标题
G（1）（τ），g（3/2）（τ）和g（2）（τ）的比较，用于布朗运动中的谐波振荡器，具有连贯的背景
A comparison of g(1)(τ), g(3/2)(τ), and g(2)(τ), for radiation from harmonic oscillators in Brownian motion with coherent background
论文作者
论文摘要
我们比较了在天体物理学中相关的模型，比较了场地G（1）（τ），强度场G（3/2）（τ）和强度 - 强度G（2）（τ）相关函数。我们获得了混乱辐射的一般情况的表达式，其中振幅是基于布朗运动中的谐波振荡器集合的模型的Rician。我们获得了两种测量方法的信号与噪声比。强度场相关函数信号与噪声比的缩放尺度为| g（1）（τ）|的第一个功率。这与g（2）（τ）的良好结果相反，后者是| g（1）（τ）|的平方。
We compare the field-field g(1)(τ), intensity-field g(3/2)(τ), and intensity-intensity g(2)(τ) correlation functions for models that are of relevance in astrophysics. We obtain expressions for the general case of a chaotic radiation, where the amplitude is Rician based on a model with an ensemble of harmonic oscillators in Brownian motion. We obtain the signal to noise ratios for two methods of measurement. The intensity-field correlation function signal to noise ratio scales with the first power of |g(1)(τ)|. This is in contrast with the well-established result of g(2)(τ) which goes as the square of |g(1)(τ)|.
