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arXiv:1601.02520 · Physical Review A

Wigner functions for the pair angle and orbital angular momentum

H.A. Kastrup

Published Dec 15, 2016• 29 citations
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Abstract

The problem of constructing physically and mathematically well-defined Wigner functions for the canonical pair angle $\ensuremath{\theta}$ and angular momentum $p$ is solved. While a key element for the construction of Wigner functions for the planar phase space ${(q,p)\ensuremath{\in}{\mathbb{R}}^{2}}$ is the Heisenberg-Weyl group, the corresponding group for the cylindrical phase space ${(\ensuremath{\theta},p)\ensuremath{\in}{S}^{1}\ifmmode\times\else\texttimes\fi{}\mathbb{R}}$ is the Euclidean group $E(2)$ of the plane and its unitary representations. Here the angle $\ensuremath{\theta}$ is replaced by the pair $(cos\ensuremath{\theta},sin\ensuremath{\theta})$, which corresponds uniquely to the points on the unit circle. The main structural properties of the Wigner functions for the planar and the cylindrical phase spaces are strikingly similar. A crucial role is played by the $sinc$ function, which provides the interpolation for the discontinuous quantized angular momenta in terms of the continuous classical ones, in accordance with the famous Whittaker cardinal function well known from interpolation and sampling theories. The quantum mechanical marginal distributions for the angle (continuous) and angular momentum (discontinuous) are, as usual, uniquely obtained by appropriate integrations of the $(\ensuremath{\theta},p)$ Wigner function. Among the examples discussed is an elementary system of simple cat states.

DOI
10.1103/physreva.94.062113

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Recently a paper on the construction of consistent Wigner functions for cylindrical phase spaces ${\mathbb{S}}^{1}\ifmmode\times\else\texttimes\fi{}\mathbb{R}$, i.e., for the canonical pair angle and orbital angular momentum, was published [H. A. Kastrup, Phys. Rev. A 94, 062113 (2016)] in which the main properties of these functions are derived and discussed and their usefulness is illustrated with examples. The present paper is a continuation which compares the properties of the Wigner functions for cylindrical phase spaces with those of the well-known Wigner functions for planar phase spaces in more detail. Furthermore, the mutual (Weyl) correspondence between Hilbert space operators and their phase-space functions is discussed. The $\ensuremath{\star}$ product formalism is shown to be completely implementable. In addition, basic dynamical laws for Wigner and Moyal functions are derived as generalized Liouville and energy equations. They are very similar to those in the planar case but also show characteristic differences.

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The problem of constructing physically and mathematically well-defined Wigner functions for the canonical pair angle \ensuremathθ\ensuremath{\theta}\ensuremathθ and angular momentum ppp is solved. While a key element for the construction of Wigner functions for the planar phase space (q,p)\ensuremath∈R2{(q,p)\ensuremath{\in}{\mathbb{R}}^{2}}(q,p)\ensuremath∈R2 is the Heisenberg-Weyl group, the corresponding group for the cylindrical phase space (\ensuremathθ,p)\ensuremath∈S1\ifmmode×\else\texttimes\fiR{(\ensuremath{\theta},p)\ensuremath{\in}{S}^{1}\ifmmode\times\else\texttimes\fi{}\mathbb{R}}(\ensuremathθ,p)\ensuremath∈S1\ifmmode×\else\texttimes\fiR is the Euclidean group E(2)E(2)E(2) of the plane and its unitary representations. Here the angle \ensuremathθ\ensuremath{\theta}\ensuremathθ is replaced by the pair (cos\ensuremathθ,sin\ensuremathθ)(cos\ensuremath{\theta},sin\ensuremath{\theta})(cos\ensuremathθ,sin\ensuremathθ), which corresponds uniquely to the points on the unit circle. The main structural properties of the Wigner functions for the planar and the cylindrical phase spaces are strikingly similar. A crucial role is played by the sincsincsinc function, which provides the interpolation for the discontinuous quantized angular momenta in terms of the continuous classical ones, in accordance with the famous Whittaker cardinal function well known from interpolation and sampling theories. The quantum mechanical marginal distributions for the angle (continuous) and angular momentum (discontinuous) are, as usual, uniquely obtained by appropriate integrations of the (\ensuremathθ,p)(\ensuremath{\theta},p)(\ensuremathθ,p) Wigner function. Among the examples discussed is an elementary system of simple cat states.
Recently a paper on the construction of consistent Wigner functions for cylindrical phase spaces ${\mathbb{S}}^{1}\ifmmode\times\else\texttimes\fi{}\mathbb{R}$, i.e., for the canonical pair angle and orbital angular momentum, was published [H. A. Kastrup, Phys. Rev. A 94, 062113 (2016)] in which the main properties of these functions are derived and discussed and their usefulness is illustrated with examples. The present paper is a continuation which compares the properties of the Wigner functions for cylindrical phase spaces with those of the well-known Wigner functions for planar phase spaces in more detail. Furthermore, the mutual (Weyl) correspondence between Hilbert space operators and their phase-space functions is discussed. The $\ensuremath{\star}$ product formalism is shown to be completely implementable. In addition, basic dynamical laws for Wigner and Moyal functions are derived as generalized Liouville and energy equations. They are very similar to those in the planar case but also show characteristic differences.
The question how to quantize a classical system where an angle $\ensuremath{\varphi}$ is one of the basic canonical variables has been controversial since the early days of quantum mechanics. The problem is that the angle is a multivalued or discontinuous variable on the corresponding phase space. The remedy is to replace $\ensuremath{\varphi}$ by the smooth periodic functions $\mathrm{cos}\phantom{\rule{0.2em}{0ex}}\ensuremath{\varphi}$ and $\mathrm{sin}\phantom{\rule{0.2em}{0ex}}\ensuremath{\varphi}$. In the case of the canonical pair $(\ensuremath{\varphi},{p}_{\ensuremath{\varphi}})$, where ${p}_{\ensuremath{\varphi}}$ is the orbital angular momentum (OAM), the phase space ${\mathcal{S}}_{\ensuremath{\varphi},{p}_{\ensuremath{\varphi}}}={\ensuremath{\varphi}∊\mathbb{R}\phantom{\rule{0.2em}{0ex}}\mathrm{mod}\phantom{\rule{0.2em}{0ex}}2\ensuremath{\pi},{p}_{\ensuremath{\varphi}}∊\mathbb{R}}$ has the global topological structure ${S}^{1}\ifmmode\times\else\texttimes\fi{}\mathbb{R}$ of a cylinder on which the Poisson brackets of the three functions $\mathrm{cos}\phantom{\rule{0.2em}{0ex}}\ensuremath{\varphi},\mathrm{sin}\phantom{\rule{0.2em}{0ex}}\ensuremath{\varphi}$, and ${p}_{\ensuremath{\varphi}}$ obey the Lie algebra of the Euclidean group E(2)\mathrm{E}(2)E(2) in the plane. This property provides the basis for the quantization of the system in terms of irreducible unitary representations of the group E(2)\mathrm{E}(2)E(2) or of its covering groups. A crucial point is that, due to the fact that the subgroup $\mathrm{SO}(2)\ensuremath{\cong}{S}^{1}$ is multiply connected, these representations allow for fractional OAM $l=\ensuremath{\hbar}(n+\ensuremath{\delta}),n∊\mathbb{Z},\ensuremath{\delta}∊[0,1)$. Such $\ensuremath{\delta}\ensuremath{\ne}0$ have already been observed in cases like the Aharonov-Bohm and fractional quantum Hall effects, and they correspond to the quasimomenta of Bloch waves in ideal crystals. The proposal of the present paper is to look for fractional OAM in connection with the quantum optics of Laguerre-Gaussian laser modes in external magnetic fields. The quantum theory of the phase space ${\mathcal{S}}_{\ensuremath{\varphi},{p}_{\ensuremath{\varphi}}}$ in terms of unitary representations of E(2)\mathrm{E}(2)E(2) allows for two types of ``coherent'' states, the properties of which are discussed in detail: nonholomorphic minimal-uncertainty states and holomorphic ones associated with Bargmann-Segal Hilbert spaces.
The framework of Wigner functions for the canonical pair angle and orbital angular momentum, derived and analyzed in 2 recent papers [H.A. Kastrup, Phys. Rev. A 94, 062113(2016) and Phys. Rev. A 95, 052111(2017)], is applied to elementary concepts of quantum information like qubits and 2-qubits, e.g., entangled EPR/Bell states etc. Properties of the associated Wigner functions are discussed and illustrated. The results may be useful for quantum information experiments with orbital angular momenta of light beams or electron beams.
The framework of Wigner functions for the canonical pair angle and orbital angular momentum, derived and analyzed in 2 recent papers [H. A. Kastrup, Phys.Rev. A 94, 062113(2016) and Phys.Rev. A 95, 052111(2017)] is applied to elementary concepts of quantum information like qubits and 2-qubits, e.g., entangled EPR/Bell states etc. Properties of the associated Wigner functions of such superposed states (pure and mixed) are discussed and illustrated. The Wigner functions of ERP/Bell states are distinguished by their topologically "twisted" domain on the configuration subspace S^1xS^1, a torus, of the total phase space. Like the applications of Wigner functions in quantum optics the results presented in the present paper may be useful for the description and analysis of quantum information experiments with orbital angular momenta of light beams or electron beams, respectively.
The Wigner distribution function is one of the pillars of the phase space formulation of quantum mechanics. Its original formulation may be cast in terms of the unitary representations of the Weyl–Heisenberg group. Following the construction proposed by Wolf and coworkers in constructing the Wigner functions for general Lie groups using the irreducible unitary representations of the groups, we develop here the Wigner functions and Weyl operators on the Euclidean motion group of rank three. We give complete derivations and proofs of their important properties.
In quantum mechanics, spatial wavefunctions describe distributions of a particle's position or momentum, but not of angular momentum jjj. In contrast, here we show that a spatial wavefunction, jm(ϕ,θ,χ)= eimϕδ(θ−θm) ei(j+1/2)χj_m (ϕ,θ,χ)=~e^{i m ϕ} δ(θ- θ_m) ~e^{i(j+1/2)χ}jm​(ϕ,θ,χ)= eimϕδ(θ−θm​) ei(j+1/2)χ, which treats jjj in the ∣jm>|jm>∣jm> state as a three-dimensional entity, is an asymptotic eigenfunction of angular-momentum operators; ϕϕϕ, θθθ, χχχ are the Euler angles, and cosθm=(m/∣j∣)cos θ_m=(m/|j|)cosθm​=(m/∣j∣) is the Vector-Model polar angle. The jm(ϕ,θ,χ)j_m (ϕ,θ,χ)jm​(ϕ,θ,χ) gives a computationally simple description of particle and orbital-angular-momentum wavepackets (constructed from Gaussian distributions in jjj and mmm) which predicts the effective wavepacket angular uncertainty relations for ΔmΔϕΔm ΔϕΔmΔϕ, ΔjΔχΔj ΔχΔjΔχ, and ΔϕΔθΔϕΔθΔϕΔθ, and the position of the particle-wavepacket angular motion on the orbital plane. The particle-wavepacket rotation can be experimentally probed through continuous and non-destructive jjj-rotation measurements. We also use the jm(ϕ,θ,χ)j_m (ϕ,θ,χ)jm​(ϕ,θ,χ) to determine well-known asymptotic expressions for Clebsch-Gordan coefficients, Wigner d-functions, the gyromagnetic ratio of elementary particles, g=2g=2g=2, and the m-state-correlation matrix elements, $$. Interestingly, for low j, even down to j=1/2j=1/2j=1/2, these expressions are either exact (the last two) or excellent approximations (the first two), showing that jm(ϕ,θ,χ)j_m (ϕ,θ,χ)jm​(ϕ,θ,χ) gives a useful spatial description of quantum-mechanical angular momentum, and provides a smooth connection with classical angular momentum.