Weak value amplification and beyond the standard quantum limit in position measurements
arXiv:1504.04777 · doi:10.1103/PhysRevA.92.032123
Abstract
In a weak measurement with post-selection, a measurement value, called the weak value, can be amplified beyond the eigenvalues of the observable. However, there are some controversies whether the weak value amplification is practically useful or not in increasing sensitivity of the measurement in which fundamental quantum noise dominates. In this paper, we investigate the sensitivity limit of an optical interferometer by properly taking account quantum shot noise and radiation pressure noise. To do so, we formulate the weak value amplification in the Heisenberg picture, which enables us to intuitively understand what happens when the measurement outcome is post-selected and the weak value is amplified. As a result, we found that the sensitivity limit is given by the standard quantum limit that is the same as in a standard interferometry. We also discuss a way to circumvent the standard quantum limit.
12 pages, 5 figures
References in corpus (6)
- Ultrasensitive Beam Deflection Measurement via Interferometric Weak Value Amplification
- Optimizing the Signal to Noise Ratio of a Beam Deflection Measurement with Interferometric Weak Values
- Entanglement-assisted weak value amplification
- Optimal Probe Wavefunction of Weak-Value Amplification
- Weak measurement: Effect of the detector dynamics
- Heisenberg scaling with weak measurement: A quantum state discrimination point of view
Cited by in corpus (5)
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- Quantum Enhanced Interferometer for Kilohertz Gravitational Wave Detection