Quantum light in the turbulent atmosphere

被引：91

作者：

Semenov, A. A. ^{[1
]}

Vogel, W. ^{[2
]}

机构：

[1] Natl Acad Sci Ukraine, Inst Phys, UA-03028 Kiev, Ukraine

[2] Univ Rostock, Inst Phys, D-18051 Rostock, Germany

来源：

PHYSICAL REVIEW A | 2009年 / 80卷 / 02期

关键词：

ELECTROMAGNETIC BEAM-PROPAGATION; SQUEEZED STATES; NOBEL LECTURE; KEY EXCHANGE; ENTANGLEMENT; HOMODYNE; RADIATION;

D O I：

10.1103/PhysRevA.80.021802

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

Nonclassical properties of light propagating through the turbulent atmosphere are studied. We demonstrate by numerical simulation that the probability distribution of the transmission coefficient, which characterizes the effects of the atmosphere on the quantum state of light, can be reconstructed by homodyne detection. Nonclassical photonstatistics and, more generally, nonclassical Glauber-Sudarshan functions appear to be more robust against turbulence for weak light fields rather than for bright ones.

引用

页数：4

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