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arXiv:2101.05889

Observables compatible to the toroidal moment operator

Dragoş-Victor Anghel, Amanda Teodora Preda

Published Jan 14, 2021• 0 citations
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Abstract

The quantum operator $\hat{T}_3$, corresponding to the projection of the toroidal moment on the $z$ axis, admits several self-adjoint extensions, when defined on the whole $\mathbb{R}^3$ space. $\hat{T}_3$ commutes with $\hat{L}_3$ (the projection of the angular momentum operator on the $z$ axis) and they have a \textit{natural set of coordinates} $(k,u,ϕ)$ where $ϕ$ is the azimuthal angle. The second set of \textit{natural coordinates} is $(k_1,k_2,u)$, where $k_1 = k\cosϕ$, $k_2 = k\sinϕ$. In both sets, $\hat{T}_3 = -i\hbar\partial/\partial u$, so any operator that is a function of $k$ and the partial derivatives with respect to the \textit{natural variables} $(k, u, ϕ)$ commute with $\hat{T}_3$ and $\hat{L}_3$. Similarly, operators that are functions of $k_1$, $k_2$, and the partial derivatives with respect to $k_1$, $k_2$, and $u$ commute with $\hat{T}_3$. Therefore, we introduce here the operators $\hat{p}_{k} \equiv -i \hbar \partial/\partial k$, $\hat{p}^{(k1)} \equiv -i \hbar \partial/\partial k_1$, and $\hat{p}^{(k2)} \equiv -i \hbar \partial/\partial k_2$ and express them in the $(x,y,z)$ coordinates. One may also invert the relations and write the typical operators, like the momentum $\hat{\bf p} \equiv -i\hbar {\bf \nabla}$ or the kinetic energy $\hat{H}_0 \equiv -\hbar^2Δ/(2m)$ in terms of the "toroidal" operators $\hat{T}_3$, $\hat{p}^{(k)}$, $\hat{p}^{(k1)}$, $\hat{p}^{(k2)}$, and, eventually, $\hat{L}_3$. The formalism may be applied to specific physical systems, like nuclei, condensed matter systems, or metamaterials. We exemplify it by calculating the momentum operator and the free particle Hamiltonian in terms of \textit{natural coordinates} in a thin torus, where the general relations get considerably simplified.

DOI
10.48550/arxiv.2101.05889

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The quantum operator T^3\hat{T}_3T^3​, corresponding to the projection of the toroidal moment on the zzz axis, admits several self-adjoint extensions, when defined on the whole R3\mathbb{R}^3R3 space. T^3\hat{T}_3T^3​ commutes with L^3\hat{L}_3L^3​ (the projection of the angular momentum operator on the zzz axis) and they have a \textit{natural set of coordinates} (k,u,ϕ)(k,u,ϕ)(k,u,ϕ) where ϕϕϕ is the azimuthal angle. The second set of \textit{natural coordinates} is (k1,k2,u)(k_1,k_2,u)(k1​,k2​,u), where k1=kcos⁡ϕk_1 = k\cosϕk1​=kcosϕ, k2=ksin⁡ϕk_2 = k\sinϕk2​=ksinϕ. In both sets, T^3=−iℏ∂/∂u\hat{T}_3 = -i\hbar\partial/\partial uT^3​=−iℏ∂/∂u, so any operator that is a function of kkk and the partial derivatives with respect to the \textit{natural variables} (k,u,ϕ)(k, u, ϕ)(k,u,ϕ) commute with T^3\hat{T}_3T^3​ and L^3\hat{L}_3L^3​. Similarly, operators that are functions of k1k_1k1​, k2k_2k2​, and the partial derivatives with respect to k1k_1k1​, k2k_2k2​, and uuu commute with T^3\hat{T}_3T^3​. Therefore, we introduce here the operators p^k≡−iℏ∂/∂k\hat{p}_{k} \equiv -i \hbar \partial/\partial kp^​k​≡−iℏ∂/∂k, p^(k1)≡−iℏ∂/∂k1\hat{p}^{(k1)} \equiv -i \hbar \partial/\partial k_1p^​(k1)≡−iℏ∂/∂k1​, and p^(k2)≡−iℏ∂/∂k2\hat{p}^{(k2)} \equiv -i \hbar \partial/\partial k_2p^​(k2)≡−iℏ∂/∂k2​ and express them in the (x,y,z)(x,y,z)(x,y,z) coordinates. One may also invert the relations and write the typical operators, like the momentum p^≡−iℏ∇\hat{\bf p} \equiv -i\hbar {\bf \nabla}p^​≡−iℏ∇ or the kinetic energy H^0≡−ℏ2Δ/(2m)\hat{H}_0 \equiv -\hbar^2Δ/(2m)H^0​≡−ℏ2Δ/(2m) in terms of the "toroidal" operators T^3\hat{T}_3T^3​, p^(k)\hat{p}^{(k)}p^​(k), p^(k1)\hat{p}^{(k1)}p^​(k1), p^(k2)\hat{p}^{(k2)}p^​(k2), and, eventually, L^3\hat{L}_3L^3​. The formalism may be applied to specific physical systems, like nuclei, condensed matter systems, or metamaterials. We exemplify it by calculating the momentum operator and the free particle Hamiltonian in terms of \textit{natural coordinates} in a thin torus, where the general relations get considerably simplified.
After a short presentation of the toroidal moments and the necessity to introduce them in the multipole expansion of current density, the correspondent quantum operators are introduced. The toroidal momentum operator (the quantum operator corresponding to the lowest-order toroidal multipole) is analysed. A natural set of coordinates is found. Using this set of coordinates it becomes possible to find the eigenvalues and a complete orthonormal set of eigenfunctions of the projection of this operator on the Oz axis.
Abstract A system of 4 point masses (without spin) is considered. The potential energy is assumed to be a function of the distances between the particles only. It is possible to express the kinetic energy relative to the center of mass as the kinetic energy of 3 "reduced" masses. The different possibilities for that procedure are discussed for systems with an arbitrary number of particles. The positions of the 3 reduced masses are described by 9 coordinates. 6 of them, the "internal" coordinates, are needed to determine the internal structure of the system, and 3, the "external" coordinates, for its orientation in space. The classical Hamiltonian in such a set of coordinates is derived. In a first step the Hamiltonian is expressed in terms of linear and angular momenta. Then these quantities are determined as functions of the coordinates and the conjugate momenta by infinitesimal trans-formations. From the classical Hamiltonian we get the quantum mechanical one by the well-known translation rule. It can be expressed in terms of the linear and angular momentum operators quite analogous to the classical case. For the solution of the time-independent Schrödinger equation the rotational symmetry of the system is used. The wave function is expanded in terms of the eigenfunctions of the total angular momentum. This leads to a system of coupled differential equations for the expansion-coefficients which depend on the 6 internal coordinates only. The further symmetries of the system (reflection and particle exchange) appear in symmetry properties of these functions. Differences and similarities in the solution theory for the 4-body-problem with respect to the 3-body-problem are discussed.
We review some of the difficulties previously encountered in defining the phase operator for finite quantum systems. We then propose the Wigner–Weyl quantization of the angle function φ on phase space as the phase operator, and derive a closed expression for its matrix elements with respect to the Hermite functions. We also determine the quantization of e^{iφ} , which turns out to be a weighted shift operator, its spectrum and that of its adjoint. This is done in the framework of quantization of a certain symbol class of phase space distributions, specialized to those which depend on one variable only. After recalling some results for the position and momentum variables, we apply the scheme to functions of radius or angle. We give necessary and sufficient conditions for operators obtained by quantizing functions of the angle to be elements of \mathscr L^+ [\mathscr S(\mathbf R)] and \mathscr L^+ [\mathscr S (\mathbf R), L^2(\mathbf R)] , and a sufficient condition for boundedness. We then consider the associated questions of commutation relations and uncertainties for operators in \mathscr L^+ [\mathscr S(\mathbf R), L^2(\mathbf R)] , which we define as bilinear forms. As must be the case, the commutator between our phase operator and the number operator exhibits noncanonical terms. Not surprisingly, the Poisson bracket of their phase space symbols also exhibits a noncanonical term.