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Physical Review

General Perturbation and Variational Methods for Responses to Time-Dependent Interactions in Quantum Mechanics

J. Heinrichs

Published Dec 25, 1968• 21 citations
Publisher
DOI
10.1103/physrev.176.2168.2

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In this chapter, we present some fundamental issues about approximation methods that are often used when a quantum-mechanical system is perturbed and about the relationship between classical and quantum mechanics. In Sec. 10.1 we introduce the stationary perturbation theory, while Sec. 10.2 is devoted to time-dependent perturbations. In Sec. 10.3 we briefly examine the adiabatic theorem. In Sec. 10.4 we introduce the variation method, an approximation method that is not based on perturbation theory. In Sec. 10.5 we discuss the classical limit of the quantum-mechanical equations, whereas in Sec. 10.6 we deal with the semiclassical approximation, in particular the WKB method. On the basis of the previous approximation methods in Sec. 10.7 we present scattering theory. Finally, in Sec. 10.8 we treat a method that has a wide range of applications: the path-integral method. Stationary perturbation theory Perturbation theory is a rather general approximation method that may be applied when a small additional force (the perturbation) acts on a system (the unperturbed system), whose quantum dynamics is fully known. If the disturbance is small, it modifies both the energy levels and the stationary states. This allows us to make an expansion in power series of a perturbation parameter, which is assumed to be small. Perturbation theory may be applied both to the case where the additional force is time-independent (in which case a stationary treatment suffices – the subject of the present section) as well as to the case where it explicitly depends on time.
The interaction between quantum matter waves and gravitational fields is a central theme in the quest to reconcile quantum mechanics with general relativity. This paper introduces the concept of a matter‑wave gravity response spectrum (MWGRS), defined as the frequency‑dependent response function χ_g(ω) that quantifies how a matter‑wave state ψ(t) reacts to temporal variations in the gravitational potential. Beginning with the Schrödinger equation in a weakly curved spacetime, we derive the linear response of the wavefunction to small metric perturbations. The response function is obtained by Fourier transforming the time‑dependent phase shift induced by the perturbation. Explicit expressions for a free particle and for a two‑path interferometer are presented, revealing how the MWGRS encodes information about both the intrinsic dynamics of the particle and the geometry of the interferometric paths. We discuss the implications of the MWGRS for upcoming precision gravimetry experiments, including its sensitivity to hypothetical spacetime foam and holographic noise. The paper concludes with a perspective on how measuring χ_g(ω) could provide a new window into the quantum structure of spacetime, potentially guiding the design of future quantum‑gravity experiments.
The interaction between quantum matter waves and gravitational fields is a central theme in the quest to reconcile quantum mechanics with general relativity. This paper introduces the concept of a matter‑wave gravity response spectrum (MWGRS), defined as the frequency‑dependent response function χ_g(ω) that quantifies how a matter‑wave state ψ(t) reacts to temporal variations in the gravitational potential. Beginning with the Schrödinger equation in a weakly curved spacetime, we derive the linear response of the wavefunction to small metric perturbations. The response function is obtained by Fourier transforming the time‑dependent phase shift induced by the perturbation. Explicit expressions for a free particle and for a two‑path interferometer are presented, revealing how the MWGRS encodes information about both the intrinsic dynamics of the particle and the geometry of the interferometric paths. We discuss the implications of the MWGRS for upcoming precision gravimetry experiments, including its sensitivity to hypothetical spacetime foam and holographic noise. The paper concludes with a perspective on how measuring χ_g(ω) could provide a new window into the quantum structure of spacetime, potentially guiding the design of future quantum‑gravity experiments.