Please use this identifier to cite or link to this item: https://doi.org/10.1103/PhysRevA.96.063829
Title: Fisher information for far-field linear optical superresolution via homodyne or heterodyne detection in a higher-order local oscillator mode
Authors: Yang, Fan
Nair, Ranjith 
Tsang, Mankei 
Simon, Christoph
Lvovsky, Alexander I
Keywords: Science & Technology
Physical Sciences
Optics
Physics, Atomic, Molecular & Chemical
Physics
LIMIT
Issue Date: 19-Dec-2017
Publisher: AMER PHYSICAL SOC
Citation: Yang, Fan, Nair, Ranjith, Tsang, Mankei, Simon, Christoph, Lvovsky, Alexander I (2017-12-19). Fisher information for far-field linear optical superresolution via homodyne or heterodyne detection in a higher-order local oscillator mode. PHYSICAL REVIEW A 96 (6). ScholarBank@NUS Repository. https://doi.org/10.1103/PhysRevA.96.063829
Abstract: The distance between two point light sources is difficult to estimate if that distance is below the diffraction (Rayleigh's) resolution limit of the imaging device. A recently proposed technique enhances the precision of this estimation by exploiting the source-separation-dependent coupling of light into higher-order transverse-electromagnetic (TEM) modes, particularly the TEM01 mode of the image. We theoretically analyze the estimation of the source separation by means of homodyne or heterodyne detection with a local oscillator in the TEM01 mode, which is maximally sensitive to the separation in the sub-Rayleigh regime. We calculate the Fisher information associated with this estimation and compare it with direct imaging. For thermal sources, the Fisher information in any mode of the image plane depends nonlinearly on the average received photon number. We show that the per-photon Fisher information surpasses that of direct imaging (in the interesting sub-Rayleigh regime) when the average received photon number per source exceeds two for homodyne detection and four for heterodyne detection.
Source Title: PHYSICAL REVIEW A
URI: https://scholarbank.nus.edu.sg/handle/10635/192273
ISSN: 24699926
24699934
DOI: 10.1103/PhysRevA.96.063829
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