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Geometric quantization

From Wikipedia, the free encyclopedia
Recipe for constructing a quantum analog of a classical physical theory

Inmathematical physics,geometric quantization is a mathematical approach to defining aquantum theory corresponding to a givenclassical theory. It attempts to carry outquantization, for which there isin general no exact recipe, in such a way that certain analogies between the classical theory and the quantum theory remain manifest. For example, the similarity between the Heisenberg equation in theHeisenberg picture ofquantum mechanics and theHamilton equation in classical physics should be built in.

Origins

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One of the earliest attempts at a natural quantization wasWeyl quantization, proposed byHermann Weyl in 1927. Here, an attempt is made to associate a quantum-mechanical observable (aself-adjoint operator on aHilbert space) with a real-valued function on classicalphase space. The position and momentum in this phase space are mapped to the generators of theHeisenberg group, and the Hilbert space appears as agroup representation of theHeisenberg group. In 1946,H. J. Groenewold considered the product of a pair of such observables and asked what the corresponding function would be on the classical phase space.[1] This led him to discover thephase-space star-product of a pair of functions.

The modern theory of geometric quantization was developed byBertram Kostant andJean-Marie Souriau in the 1970s. One of the motivations of the theory was to understand and generalize Kirillov'sorbit method in representation theory.

Types

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The geometric quantization procedure falls into the following three steps: prequantization, polarization, and metaplectic correction. Prequantization produces a natural Hilbert space together with a quantization procedure for observables that exactly transforms Poisson brackets on the classical side into commutators on the quantum side. Nevertheless, the prequantum Hilbert space is generally understood to be "too big".[2] The idea is that one should then select a Poisson-commuting set ofn variables on the 2n-dimensional phase space and consider functions (or, more properly, sections) that depend only on thesen variables. Then variables can be either real-valued, resulting in a position-style Hilbert space, or complex analytic, producing something like theSegal–Bargmann space.[a]A polarization is a coordinate-independent description of such a choice ofn Poisson-commuting functions. The metaplectic correction (also known as the half-form correction) is a technical modification of the above procedure that is necessary in the case of real polarizations and often convenient for complex polarizations.

Prequantization

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Suppose(M,ω){\displaystyle (M,\omega )} is a symplectic manifold with symplectic formω{\displaystyle \omega }. Suppose at first thatω{\displaystyle \omega } is exact, meaning that there is a globally definedsymplectic potentialθ{\displaystyle \theta } withdθ=ω{\displaystyle d\theta =\omega }. We can consider the "prequantum Hilbert space" of square-integrable functions onM{\displaystyle M} (with respect to the Liouville volume measure). For each smooth functionf{\displaystyle f} onM{\displaystyle M}, we can define the Kostant–Souriau prequantum operator

Q(f):=i(Xf+1iθ(Xf))+f{\displaystyle Q(f):=-i\hbar \left(X_{f}+{\frac {1}{i\hbar }}\theta (X_{f})\right)+f}.

whereXf{\displaystyle X_{f}} is the Hamiltonian vector field associated tof{\displaystyle f}.

More generally, suppose(M,ω){\displaystyle (M,\omega )} has the property that the integral ofω/(2π){\displaystyle \omega /(2\pi \hbar )} over any closed surface is an integer. Then we can construct a line bundleL{\displaystyle L} with connection whose curvature 2-form isω/{\displaystyle \omega /\hbar }. In that case, the prequantum Hilbert space is the space of square-integrable sections ofL{\displaystyle L}, and we replace the formula forQ(f){\displaystyle Q(f)} above with

Q(f)=iXf+f{\displaystyle Q(f)=-i\hbar \nabla _{X_{f}}+f},

with{\displaystyle \nabla } the connection.The prequantum operators satisfy

[Q(f),Q(g)]=iQ({f,g}){\displaystyle [Q(f),Q(g)]=i\hbar Q(\{f,g\})}

for all smooth functionsf{\displaystyle f} andg{\displaystyle g}.[3]

The construction of the preceding Hilbert space and the operatorsQ(f){\displaystyle Q(f)} is known asprequantization.

Polarization

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The next step in the process of geometric quantization is the choice of a polarization. A polarization is a choice at each point inM{\displaystyle M} a Lagrangian subspace of the complexified tangent space ofM{\displaystyle M}. The subspaces should form an integrable distribution, meaning that the commutator of two vector fields lying in the subspace at each point should also lie in the subspace at each point. Thequantum (as opposed to prequantum) Hilbert space is the space of sections ofL{\displaystyle L} that are covariantly constant in the direction of the polarization.[4][b]The idea is that in the quantum Hilbert space, the sections should be functions of onlyn{\displaystyle n} variables on the2n{\displaystyle 2n}-dimensional classical phase space.

Iff{\displaystyle f} is a function for which the associated Hamiltonian flow preserves the polarization, thenQ(f){\displaystyle Q(f)} will preserve the quantum Hilbert space.[5]The assumption that the flow off{\displaystyle f} preserve the polarization is a strong one. Typically, not very many functions will satisfy this assumption.

Half-form correction

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The half-form correction—also known as the metaplectic correction—is a technical modification to the above procedure that is necessary in the case of real polarizations to obtain a nonzero quantum Hilbert space; it is also often useful in the complex case. The line bundleL{\displaystyle L} is replaced by the tensor product ofL{\displaystyle L} with the square root of the canonical bundle of the polarization. In the case of the vertical polarization, for example, instead of considering functionsf(x){\displaystyle f(x)} ofx{\displaystyle x} that are independent ofp{\displaystyle p}, one considers objects of the formf(x)dx{\displaystyle f(x){\sqrt {dx}}}. The formula forQ(f){\displaystyle Q(f)} must then be supplemented by an additional Lie derivative term.[6]In the case of a complex polarization on the plane, for example, the half-form correction allows the quantization of the harmonic oscillator to reproduce the standard quantum mechanical formula for the energies,(n+1/2)ω{\displaystyle (n+1/2)\hbar \omega }, with the "+1/2{\displaystyle +1/2}" coming courtesy of the half-forms.[7]

Poisson manifolds

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Geometric quantization of Poisson manifolds and symplectic foliations also is developed. For instance, this is the case ofpartially integrable andsuperintegrable Hamiltonian systems andnon-autonomous mechanics.

Example

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In the case that the symplectic manifold is the2-sphere, it can be realized as acoadjoint orbit insu(2){\displaystyle {\mathfrak {su}}(2)^{*}}. Assuming that the area of the sphere is an integer multiple of2π{\displaystyle 2\pi \hbar }, we can perform geometric quantization and the resulting Hilbert space carries an irreducible representation ofSU(2). In the case that the area of the sphere is2π{\displaystyle 2\pi \hbar }, we obtain the two-dimensionalspin-1/2 representation.

Generalization

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More generally, this technique leads todeformation quantization, where the ★-product is taken to be a deformation of the algebra of functions on asymplectic manifold orPoisson manifold. However, as a natural quantization scheme (a functor), Weyl's map is not satisfactory. For example, the Weyl map of the classical angular-momentum-squared is not just the quantum angular momentum squared operator, but it further contains a constant term 3ħ2/2. (This extra term is actually physically significant, since it accounts for the nonvanishing angular momentum of the ground-state Bohr orbit in the hydrogen atom.[8]) As a mere representation change, however, Weyl's map underlies the alternatephase-space formulation of conventional quantum mechanics.

See also

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Notes

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  1. ^SeeHall 2013, Section 22.4 for simple examples.
  2. ^See Section 22.4 ofHall 2013 for examples in the Euclidean case.

Citations

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  1. ^Groenewold 1946, pp. 405–460.
  2. ^Hall 2013, Section 22.3.
  3. ^Hall 2013, Theorem 23.14.
  4. ^Hall 2013, Section 23.4.
  5. ^Hall 2013, Theorem 23.24.
  6. ^Hall 2013, Sections 23.6 and 23.7.
  7. ^Hall 2013, Example 23.53.
  8. ^Dahl & Schleich 2002.

Sources

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External links

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