Beyond the diffraction limit via optical amplification

被引:15
作者
Kellerer, Aglae N. [1 ]
Ribak, Erez N. [2 ]
机构
[1] Univ Cambridge, Cavendish Lab, Cambridge CB2 1TN, England
[2] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel
关键词
QUANTUM; FLUCTUATIONS; ALWAYS; CANNOT; NOISE;
D O I
10.1364/OL.41.003181
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
In a previous article [Astron. Astrophys. 561, A118 (2014)], we suggested a method to overcome the diffraction limit behind a telescope. We discuss and extend recent numerical simulations and test whether it is indeed possible to use photon amplification to enhance the angular resolution of a telescope or a microscope beyond the diffraction limit. An essential addition is the proposal to select events with an above-average ratio of stimulated to spontaneous photons. The analysis shows that the diffraction limit of a telescope is surpassed by a factor of 10 for an amplifier gain of 200, if the analysis is restricted to a tenth of the incoming astronomical photons. A gain of 70 is sufficient with a hundredth of the photons. More simulations must be performed to account for the bunching of spontaneous photons. (C) 2016 Optical Society of America
引用
收藏
页码:3181 / 3184
页数:4
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