Three Alternative Model-Building Strategies Using Quasi-Hermitian Time-Dependent Observables

Abstract

In the conventional (so-called Schrodinger-picture) formulation of quantum theory the operators of observables are chosen self-adjoint and time-independent. In the recent innovation of the theory, the operators can be not only non-Hermitian but also time-dependent. The formalism (called non-Hermitian interaction-picture, NIP) requires a separate description of the evolution of the time-dependent states ? (t) (using Schrodinger-type equations) as well as of the time-dependent observables A(j)(t), j = 1, 2, ... , K (using Heisenberg-type equations). In the unitary-evolution dynamical regime of our interest, both of the respective generators of the evolution (viz., in our notation, the Schrodingerian generator Sigma(t) and the Heisenbergian generator S(t)) have, in general, complex spectra. Only the spectrum of their superposition remains real. Thus, only the observable superposition H(t) = G(t) + Sigma(t) (representing the instantaneous energies) should be called Hamiltonian. In applications, nevertheless, the mathematically consistent models can be based not only on the initial knowledge of the energy operator Sigma(t) (forming a "dynamical" model-building strategy) but also, alternatively, on the knowledge of the Coriolis force S(t) (forming a "kinematical" model-building strategy), or on the initial knowledge of the Schrodingerian generator G(t) (forming, for some reason, one of the most popular strategies in the literature). In our present paper, every such choice (marked as "one", "two" or "three", respectively) is shown to lead to a construction recipe with a specific range of applicability.