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Directly measuring mean and variance of infinite-spectrum observables such as the photon orbital angular momentum

机译:直接测量无限光谱可观测值的均值和方差例如光子轨道角动量

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摘要

The standard method for experimentally determining the probability distribution of an observable in quantum mechanics is the measurement of the observable spectrum. However, for infinite-dimensional degrees of freedom, this approach would require ideally infinite or, more realistically, a very large number of measurements. Here we consider an alternative method which can yield the mean and variance of an observable of an infinite-dimensional system by measuring only a two-dimensional pointer weakly coupled with the system. In our demonstrative implementation, we determine both the mean and the variance of the orbital angular momentum of a light beam without acquiring the entire spectrum, but measuring the Stokes parameters of the optical polarization (acting as pointer), after the beam has suffered a suitable spin–orbit weak interaction. This example can provide a paradigm for a new class of useful weak quantum measurements.
机译:通过实验确定量子力学中可观察物的概率分布的标准方法是测量可观察光谱。但是,对于无限维的自由度,此方法将理想地需要无限或更实际地非常大量的测量。在这里,我们考虑另一种方法,该方法可以通过仅测量与系统弱耦合的二维指针来得出无限维系统的可观测值的均值和方差。在我们的演示性实现中,我们确定光束的轨道角动量的均值和方差,而无需获取整个光谱,而是在光束经受了适当的测量之后,测量光偏振的斯托克斯参数(充当指针)自旋轨道弱相互作用。这个例子可以为一类新的有用的弱量子测量提供范例。

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