Nonclassical light explained

Nonclassical light is light that cannot be described using classical electromagnetism; its characteristics are described by the quantized electromagnetic field and quantum mechanics.

The most common described forms of nonclassical light are the following:

Glauber–Sudarshan P representation

See main article: Glauber–Sudarshan P representation. The density matrix for any state of light can be written as:

\widehat{\rho}=\intP(\alpha)|{\alpha}\rangle\langle{\alpha}|\rm{d}2\alpha,

where

\scriptstyle|\alpha\rangle

is a coherent state. A classical state of light is one in which

\scriptstyleP(\alpha)

is a probability density function. If it is not, the state is said to be nonclassical.

Aspects of

\scriptstyleP(\alpha)

that would make it nonclassical are:

The matter is not quite simple. According to Mandel and Wolf: "The different coherent states are not [mutually] orthogonal, so that even if

\scriptstyleP(\alpha)

behaved like a true probability density [function], it would not describe probabilities of mutually exclusive states."

References

General references

Notes and References

  1. M. Fox, Quantum Optics: An Introduction, Oxford University Press, New York, 2006