Wigner–Weyl transform
In quantum mechanics, the Wigner–Weyl transform or Weyl–Wigner transform is the invertible mapping between functions in the quantum phase space formulation and Hilbert space operators in the Schrödinger picture.
Often the mapping from functions on phase space to operators is called the Weyl transform or Weyl quantization, whereas the inverse mapping, from operators to functions on phase space, is called the Wigner transform. This mapping was originally devised by Hermann Weyl in 1927 in an attempt to map symmetrized classical phase space functions to operators, a procedure known as Weyl quantization. It is now understood that Weyl quantization does not satisfy all the properties one would require for quantization and therefore sometimes yields unphysical answers. On the other hand, some of the nice properties described below suggest that if one seeks a single consistent quantization procedure mapping functions on the classical phase space to operators, the Weyl quantization is the best option.
Regardless, the Weyl–Wigner transform is a well-defined integral transform between the phase-space and operator representations, and yields insight into the workings of quantum mechanics. Most importantly, the Wigner quasi-probability distribution is the Wigner transform of the quantum density matrix, and, conversely, the density matrix is the Weyl transform of the Wigner function.
In contrast to Weyl's original intentions in seeking a consistent quantization scheme, this map merely amounts to a change of representation within quantum mechanics; it need not connect "classical" with "quantum" quantities. For example, the phase-space function may depend explicitly on Planck's constant ħ, as it does in some familiar cases involving angular momentum. This invertible representation change then allows one to express quantum mechanics in phase space, as was appreciated in the 1940s by Hilbrand J. Groenewold and José Enrique Moyal.
Definition of the Weyl quantization of a general observable
The following explains the Weyl transformation on the simplest, two-dimensional Euclidean phase space. Let the coordinates on phase space be, and let be a function defined everywhere on phase space. In what follows, we fix operators P and Q satisfying the canonical commutation relations, such as the usual position and momentum operators in the Schrödinger representation. We assume that the exponentiated operators and constitute an irreducible representation of the Weyl relations, so that the Stone–von Neumann theorem holds.The basic formula
The Weyl transform of the function is given by the following operator in Hilbert space,Throughout, is the reduced Planck constant.
It is instructive to perform the p and q integrals in the above formula first, which has the effect of computing the ordinary Fourier transform of the function, while leaving the operator. In that case, the Weyl transform can be written as
We may therefore think of the Weyl map as follows: We take the ordinary Fourier transform of the function, but then when applying the Fourier inversion formula, we substitute the quantum operators and for the original classical variables and, thus obtaining a "quantum version of."
A less symmetric form, but handy for applications, is the following,
In the position representation
The Weyl map may then also be expressed in terms of the integral kernel matrix elements of this operator,The inverse map
The inverse of the above Weyl map is the Wigner map, which takes the operator back to the original phase-space kernel function,If one replaces in the above expression with an arbitrary operator, the resulting function may depend on Planck's constant, and may well describe quantum-mechanical processes, provided it is properly composed through the star product, below.
In turn, the Weyl map of the Wigner map is summarized by Groenewold's formula,
The Weyl quantization of polynomial observables
While the above formulas give a nice understanding of the Weyl quantization of a very general observable on phase space, they are not very convenient for computing on simple observables, such as those that are polynomials in and. In later sections, we will see that on such polynomials, the Weyl quantization represents the totally symmetric ordering of the noncommuting operators and.For example, the Wigner map of the quantum angular-momentum-squared operator L2 is not just the classical angular momentum squared, but it further contains an offset term , which accounts for the nonvanishing angular momentum of the ground-state Bohr orbit.
Properties
Weyl quantization of polynomials
The action of the Weyl quantization on polynomial functions of and is completely determined by the following symmetric formula:for all complex numbers and. From this formula, it is not hard to show that the Weyl quantization on a function of the form gives the average of all possible orderings of factors of and factors of.
For example, we have
While this result is conceptually natural, it is not convenient for computations when and are large. In such cases, we can use instead McCoy's formula
This expression gives an apparently different answer for the case of from the totally symmetric expression above. There is no contradiction, however, since the canonical commutation relations allow for more than one expression for the same operator.
It is widely thought that the Weyl quantization, among all quantization schemes, comes as close as possible to mapping the Poisson bracket on the classical side to the commutator on the quantum side. For example,
Weyl quantization of general functions
- If is a real-valued function, then its Weyl-map image is self-adjoint.
- If is an element of Schwartz space, then is trace-class.
- More generally, is a densely defined unbounded operator.
- The map is one-to-one on the Schwartz space.
Deformation quantization
Here, it provides rules for how to deform the "classical" commutative algebra of observables to a quantum non-commutative algebra of observables.
The basic setup in deformation theory is to start with an algebraic structure and ask: Does there exist a one or more parameter family of similar structures, such that for an initial value of the parameter one has the same structure one started with? E.g., one may define a noncommutative torus as a deformation quantization through a ★-product to implicitly address all convergence subtleties. Insofar as the algebra of functions on a space determines the geometry of that space, the study of the star product leads to the study of a non-commutative geometry deformation of that space.
In the context of the above flat phase-space example, the star product, ★ħ, of a pair of functions in , is specified by
The star product is not commutative in general, but goes over to the ordinary commutative product of functions in the limit of . As such, it is said to define a deformation of the commutative algebra of.
For the Weyl-map example above, the ★-product may be written in terms of the Poisson bracket as
Here, Π is the Poisson bivector, an operator defined such that its powers are
and
where is the Poisson bracket. More generally,
where is the binomial coefficient.
Thus, e.g., Gaussians compose hyperbolically,
or
etc.
These formulas are predicated on coordinates in which the Poisson bivector is constant. For the general formula on arbitrary Poisson manifolds, cf. the Kontsevich quantization formula.
Antisymmetrization of this ★-product yields the Moyal bracket, the proper quantum deformation of the Poisson bracket, and the phase-space isomorph of the quantum commutator in the more usual Hilbert-space formulation of quantum mechanics. As such, it provides the cornerstone of the dynamical equations of observables in this phase-space formulation.
There results a complete phase space formulation of quantum mechanics, completely equivalent to the Hilbert-space operator representation, with star-multiplications paralleling operator multiplications isomorphically.
Expectation values in phase-space quantization are obtained isomorphically to tracing operator observables with the density matrix in Hilbert space: they are obtained by phase-space integrals of observables such as the above with the Wigner quasi-probability distribution effectively serving as a measure.
Thus, by expressing quantum mechanics in phase space, the above Weyl map facilitates recognition of quantum mechanics as a deformation of classical mechanics, with deformation parameter.
Classical expressions, observables, and operations are modified by -dependent quantum corrections, as the conventional commutative multiplication applying in classical mechanics is generalized to the noncommutative star-multiplication characterizing quantum mechanics and underlying its uncertainty principle.
Despite its name, Deformation Quantization does not constitute a successful quantization scheme, namely a method to produce a quantum theory out of a classical one. It amounts to a mere representation change from Hilbert space to phase space.