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In Physics , the canonical commutation relation is the relation

: {Link without Title} = i\hbar

among the position x and momentum p of a point particle in one dimension, where {Link without Title} =xp-px is the so-called Commutator of x and p, i is the Imaginary Unit and \hbar is the reduced Planck's Constant h/2\pi. This relation is attributed to Heisenberg , and it implies his Uncertainty Principle .


RELATION TO CLASSICAL MECHANICS


By contrast, in Classical Physics all observables commute and the Commutator would be zero; however, an analogous relation exists, which is obtained by replacing the commutator with the Poisson Bracket and the constant i\hbar with 1:

:\{x,p\} = 1

This observation led Dirac to postulate that, in general, the quantum counterparts \hat f,\hat g of classical observables f,g should satisfy

: f,\hat g = i\hbar\widehat{\{f,g\}}.\,

In 1927 , Hermann Weyl showed that a literal correspondence between a quantum operator and a classical distribution in Phase Space could not hold. However, he did propose a mechanism, Weyl Quantization , that underlies a mathematical approach to quantization known as Deformation Quantization .


REPRESENTATIONS


According to the standard Mathematical Formulation Of Quantum Mechanics , quantum observables such as x and p should be represented as Self-adjoint Operator s on some Hilbert Space . It is relatively easy to see that two Operator s satisfying the canonical commutation relations cannot both be Bounded . The canonical commutation relations can be made tamer by writing them in terms of the (bounded) Unitary Operator s e^{-ikx} and e^{-iap}. The result is the so-called Weyl Relations . The uniqueness of the canonical commutation relations between position and momentum is guaranteed by the Stone-von Neumann Theorem . The Group associated with the commutation relations is called the Heisenberg Group .


GENERALIZATIONS


The simple formula

: {Link without Title} = i\hbar,

valid for the Quantization of the simplest classical system, can be generalized to the case of an arbitrary Lagrangian {\mathcal L}. We identify canonical coordinates (such as x in the example above, or a field \phi(x) in the case of Quantum Field Theory ) and '''canonical momenta''' \pi_x (in the example above it is p, or more generally, some functions involving the Derivative s of the canonical coordinates with respect to time).

:\pi_i \equiv rac{\partial {\mathcal L}}{\partial(\partial x_i / \partial t)}

This definition of the canonical momentum ensures that one of the Euler-Lagrange Equation s has the form

: rac{\partial}{\partial t} \pi_i = rac{\partial {\mathcal L}}{\partial x_i}

The canonical commutation relations then say

: {Link without Title} = i\hbar\delta_{ij}

where \delta_{ij} is the Kronecker Delta .


SEE ALSO