Nonclassical light

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

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

Glauber–Sudarshan P representation

The density matrix for any state of light can be written as:

where is a coherent state. A classical state of light is one in which is a probability density function. If it is not, the state is said to be nonclassical. [2]

Aspects of 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 behaved like a true probability density [function], it would not describe probabilities of mutually exclusive states." [2]

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Squeezed states of light Quantum states light can be in

In quantum physics, light is in a squeezed state if its electric field strength Ԑ for some phases has a quantum uncertainty smaller than that of a coherent state. The term squeezing thus refers to a reduced quantum uncertainty. To obey Heisenberg's uncertainty relation, a squeezed state must also have phases at which the electric field uncertainty is anti-squeezed, i.e. larger than that of a coherent state. Since 2019, the gravitational-wave observatories LIGO and Virgo employ squeezed laser light, which has significantly increased the rate of observed gravitational-wave events.

References

Citations

  1. M. Fox, Quantum Optics: An Introduction, Oxford University Press, New York, 2006
  2. 1 2 Mandel & Wolf 1995 , p. 541


Citation bibliography

Mandel, L.; Wolf, E. (1995), Optical Coherence and Quantum Optics, Cambridge UK: Cambridge University Press, ISBN   0-521-41711-2

General references