A New Look at the Quantum Mechanics of the Harmonic Oscillator
H. A. Kastrup
Abstract
Classically the Harmonic Oscillator (HO) is the generic example for the use of angle and action variables phi in R mod 2 pi and I > 0. But the symplectic transformation (ϕ,I) to (q,p) is singular for (q,p) = (0,0). Globally (q,p) has the structure of the plane R2, but (phi,I) that of the punctured plane R2 -(0,0). This implies qualitative differences for the QM of the two phase spaces: The quantizing group for the plane R2 consists of the (centrally extended) translations generated by q,p,1, but the corresponding group for (phi,I) is SO(1,2) = Sp(2,R)/Z2, (Sp(2,R): symplectic group of the plane), with Lie algebra basis h0 = I, h1 = I cos phi, h2 = - I sin phi. In the QM for the (phi,I)-model the three hj correspond to self-adjoint generators Kj, j=0,1,2, of irreducible unitary representations (positive discrete series) for SO(1,2) or one of its infinitely many covering groups, the Bargmann index k > 0 of which determines the ground state energy E (k, n=0) = hbar omega k of the (phi,I)-Hamiltonian H(K). For an m-fold covering the lowest possible value is k=1/m, which can be made arbitrarily small! The operators Q and P, now expressed as functions of the Kj, keep their usual properties, but the richer structure of the Kj quantum model of the HO is ``erased'' when passing to the simpler Q,P model! The (phi,I)-variant of the HO implies many experimental tests: Mulliken-type experiments for isotopic diatomic molecules, experiments with harmonic traps for atoms, ions and BE-condensates, with the (Landau) levels of charged particles in magnetic fields, with the propagation of light in vacuum, passing through electric or magnetic fields. Finally it leads to a new theoretical estimate for the quantum vacuum energy of fields and its relation to the cosmological constant.
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