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Physical Review

The Torsion Oscillator-Rotator in the Quantum Mechanics

Harald H. Nielsen

Published May 1, 1932• 147 citations
Publisher

Abstract

The theory of a symmetric rotator which in addition to the usual three degrees of rotational freedom has about the axis of symmetry also a degree of torsional freedom between two of its principal parts, is treated quantum mechanically. The potential energy is taken to be expressible in the form: $V=L(1\ensuremath{-}cosm{\ensuremath{\varphi}}^{\ensuremath{'}})$ where $L$ is proportional to the restoring torque, ${\ensuremath{\varphi}}^{\ensuremath{'}}$ is the angle of displacement, and $m$ the number of minima of the potential energy curve as ${\ensuremath{\varphi}}^{\ensuremath{'}}$ increases from zero to $2\ensuremath{\pi}$. The Schr\"odinger equation is found to be separable into two differential equations, one being the quantum mechanical equation for an ordinary symmetric rotator, and the other being of the form of Mathieu's equation: $\frac{{d}^{2}M}{d{x}^{2}}+(a+16qcos2x)$ $M=0$ in which $a$ is proportional to the energy parameter of the oscillator, $q$ proportional to the restoring torque, and $x$ to ${\ensuremath{\varphi}}^{\ensuremath{'}}$. It is found that the solutions to this equation must satisfy the condition: $M(x\ensuremath{-}m\ensuremath{\pi})=(\mathrm{exp}\ensuremath{-}\frac{2\ensuremath{\pi}\mathrm{iK}{{A}_{z}}^{\ensuremath{'}}}{{A}_{z}}) M(x)$ where $K$ is the quantum number of angular momentum about the axis of symmetry, ${{A}_{z}}^{\ensuremath{'}}$ and ${A}_{z}$ the moments of inertia of the lower part of the top and of the whole of the top respectively about the axis of symmetry. This ordinarily demands a general non-periodic solution to Mathieu's equation which, however, degenerates like the ordinary Mathieu functions to an exponential function as $q\ensuremath{\rightarrow}0$. A qualitative discussion is given about the manner in which the energy states in the limiting case where $q=0$ go over into the other limiting case where $q=\ensuremath{\infty}$, and the calculation of the intensities and the selection rules for the rotator are finally determined where $q=0$ and where $q=\ensuremath{\infty}$. These it is believed will also be valid at least in first approximation in the neighborhoods of these limiting cases where $q$ no longer is quite zero and not quite equal to infinity.

DOI
10.1103/physrev.40.445

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The theory of a symmetric rotator which in addition to the usual three degrees of rotational freedom has about the axis of symmetry also a degree of torsional freedom between two of its principal parts, is treated quantum mechanically. The potential energy is taken to be expressible in the form: V=L(1\ensuremath−cosm\ensuremathφ\ensuremath′)V=L(1\ensuremath{-}cosm{\ensuremath{\varphi}}^{\ensuremath{'}})V=L(1\ensuremath−cosm\ensuremathφ\ensuremath′) where LLL is proportional to the restoring torque, \ensuremathφ\ensuremath′{\ensuremath{\varphi}}^{\ensuremath{'}}\ensuremathφ\ensuremath′ is the angle of displacement, and mmm the number of minima of the potential energy curve as \ensuremathφ\ensuremath′{\ensuremath{\varphi}}^{\ensuremath{'}}\ensuremathφ\ensuremath′ increases from zero to 2\ensuremathπ2\ensuremath{\pi}2\ensuremathπ. The Schr"odinger equation is found to be separable into two differential equations, one being the quantum mechanical equation for an ordinary symmetric rotator, and the other being of the form of Mathieu's equation: d2Mdx2+(a+16qcos2x)\frac{{d}^{2}M}{d{x}^{2}}+(a+16qcos2x)dx2d2M​+(a+16qcos2x) M=0M=0M=0 in which aaa is proportional to the energy parameter of the oscillator, qqq proportional to the restoring torque, and xxx to \ensuremathφ\ensuremath′{\ensuremath{\varphi}}^{\ensuremath{'}}\ensuremathφ\ensuremath′. It is found that the solutions to this equation must satisfy the condition: M(x\ensuremath−m\ensuremathπ)=(exp\ensuremath−2\ensuremathπiKAz\ensuremath′Az)M(x)M(x\ensuremath{-}m\ensuremath{\pi})=(\mathrm{exp}\ensuremath{-}\frac{2\ensuremath{\pi}\mathrm{iK}{{A}_{z}}^{\ensuremath{'}}}{{A}_{z}}) M(x)M(x\ensuremath−m\ensuremathπ)=(exp\ensuremath−Az​2\ensuremathπiKAz​\ensuremath′​)M(x) where KKK is the quantum number of angular momentum about the axis of symmetry, Az\ensuremath′{{A}_{z}}^{\ensuremath{'}}Az​\ensuremath′ and Az{A}_{z}Az​ the moments of inertia of the lower part of the top and of the whole of the top respectively about the axis of symmetry. This ordinarily demands a general non-periodic solution to Mathieu's equation which, however, degenerates like the ordinary Mathieu functions to an exponential function as q\ensuremath→0q\ensuremath{\rightarrow}0q\ensuremath→0. A qualitative discussion is given about the manner in which the energy states in the limiting case where q=0q=0q=0 go over into the other limiting case where q=\ensuremath∞q=\ensuremath{\infty}q=\ensuremath∞, and the calculation of the intensities and the selection rules for the rotator are finally determined where q=0q=0q=0 and where q=\ensuremath∞q=\ensuremath{\infty}q=\ensuremath∞. These it is believed will also be valid at least in first approximation in the neighborhoods of these limiting cases where qqq no longer is quite zero and not quite equal to infinity.
Schr\"odinger's method for determining the energy levels of an atomic system is applied to the case of the symmetrical top (moment of inertia about axis of symmetry CCC, the other one AAA). The energy values are found to be ${W}_{\mathrm{jn}}=\frac{{h}^{2}}{8{\ensuremath{\pi}}^{2}}\left[\frac{1}{A}j(j+1)+\left(\frac{1}{C}\ensuremath{-}\frac{1}{A}\right){n}^{2}\right]$ in agreement with the result obtained by Dennison from the matrix mechanics. The quantum numbers jjj and nnn must be integers restricted by $0\ensuremath{\leqq}j$, $|n|\ensuremath{\leqq}j$, while half-integral values are not permissible. The intensities of transitions are also calculated.
It is well known that in classical mechanics algebraic integrals of the top equations only exist in the cases of Euler (asymmetric top, no electric moment), of Lagrange (symmetric top, electric moment parallel to the axis of figure) and of Kowalewski. The latter case is that of a symmetric top whose two equal moments of inertia are twice as large as the third (A=B=2CA=B=2CA=B=2C) with an electric moment perpendicular to the axis of figure. The quantum mechanical analogue to Euler's and Lagrange's cases being well known, Kowalewski's case was tried. If $\ensuremath{\vartheta}$, $\ensuremath{\psi}$, $\ensuremath{\phi}$ are the Euler angles, QI=Q1+iQ2{Q}_{\mathrm{I}}={Q}_{1}+i{Q}_{2}QI​=Q1​+iQ2​, ${Q}_{\mathrm{II}}={Q}_{1}\ensuremath{-}i{Q}_{2}$ linear combinations of the momenta around the principal axes and $U={{Q}_{\mathrm{I}}}^{2}+4C\ensuremath{\mu}sin\ensuremath{\vartheta}{e}^{\ensuremath{-}i\ensuremath{\psi}},$ then Kowalewski's integral becomes: UU∗+U∗U+4h2(QIQII+QIIQI)=Diag.Matrix,U{U}^{*}+{U}^{*}U+4{h}^{2}({Q}_{\mathrm{I}}{Q}_{\mathrm{II}}+{Q}_{\mathrm{II}}{Q}_{\mathrm{I}})=\mathrm{Diag}.\mathrm{Matrix},UU∗+U∗U+4h2(QI​QII​+QII​QI​)=Diag.Matrix, which differs from the classical result by the symmetrization and by the last term proportional to h2{h}^{2}h2.
The states of a planar oscillator are separated to a vibrational mode, containing a zero-point energy, and a rotational mode without the zero-point energy, but having a conserved angular momentum.On the basis of the analysis of properties of models of rigid and semirigid rotators, the theory of soft rotators is formulated where the harmonic attractive force is balanced only by the centrifugal force.As examples a Coulomb rotator (the Bohr model) and a magneto-harmonic rotator (the Fock-Landau levels) are considered.Disappearance of the radial speed in the model of a magneto-harmonic rotator is taken as a defining property of a pure rotational motion in the harmonic potential.After the exception of energies of the magnetic and spin decompositions, specific to magnetic fields, one turns to a simple and general model of a plane harmonic rotator (circular oscillator without radial speed) where kinetic energy is reduced to the purely rotational energy.Energy levels of the harmonic rotator have the same frequency and are twice degenerate, the energy spectrum is equidistant.In the ground state there is no zeropoint energy from rotational modes, and the zero-point energy of vibrational modes can be compensated by spin effects or symmetries of the system.In this case the operators of observables vanish the ground state, i.e. are "strongly" normally ordered.In a chain of harmonic rotators collective rotations around a common axis lead to transverse waves, at quantization of which there appear quasi-particles and holes carrying an angular momentum.In the chain SU (2) appears as a group of symmetry of a rotator.
A semianalytical approach to the quantum dynamics of a plane pendulum is developed, based on Mathieu functions which appear as stationary wave functions. The time-dependent Schr\"odinger equation is solved for pendular analogs of coherent and squeezed states of a harmonic oscillator, induced by instantaneous changes of the periodic potential energy function. Coherent pendular states are discussed between the harmonic limit for small displacements and the inverted pendulum limit, while squeezed pendular states are shown to interpolate between vibrational and free rotational motion. In the latter case, full and fractional revivals as well as spatiotemporal structures in the time evolution of the probability densities (quantum carpets) are quantitatively analyzed. Corresponding expressions for the mean orientation are derived in terms of Mathieu functions in time. For periodic double well potentials, different revival schemes, and different quantum carpets are found for the even and odd initial states forming the ground tunneling doublet. Time evolution of the mean alignment allows the separation of states with different parity. Implications for external (rotational) and internal (torsional) motion of molecules induced by intense laser fields are discussed.
\n We have formulated a model of a complex (two-dimensional) quantum harmonic oscillator. All dynamical physical variables are expressed in terms of the creation and annihilation operators, viz., $a_{z}, \\bar{a}_{z}\\ {\\rm and} \\ a_{\\bar{z}}, \\bar{a}_{\\bar{z}} $. The Hamiltonian of the system is $H_{z\\bar{z}} = (\\bar{a}_{z}a_{z} + 1) + \\omega L_{z} $, where ω is the oscillator frequency and $L_{z} = \\frac{\\hbar }{2}\\,(\\bar{a}_{\\bar{z}} a_{\\bar{z}}-\\bar{a}_{z}a_{z}) $ is the orbital angular momentum. The oscillator is found to be described by a conserved orbital angular momentum (Lz) besides energy. While the ground-state wave function is real, all excited states are complex and degenerate. The oscillator in these states carry a quantum of charge of $e^{{\\ast}} = \\frac{n}{2n\\pm1} e $. These degenerate wave functions are eigenstates of the orbital angular momentum with eigenvalues nℏ and −nℏ, where h=2πℏ is the Planck's constant and n=1, 2, … . The two wave functions are degenerate with energy En=(n+1)ℏω. The comparison with Landau level reveals that in the presence of the magnetic field, B, where ω is equal to the cyclotron frequency, the current moment is quantized and is proportional to the square root of the magnetic field, i.e., ${\\cal I}_{n}\\propto n e \\sqrt{B} $.\n