Shapiro's plane waves in spaces of constant curvature and separation of variables in real and complex coordinates

Abstract

The aim of the article to clarify the status of Shapiro plane wave solutions of the Schrödinger's equation in the frames of the well-known general method of separation of variables. To solve this task, we use the well-known cylindrical coordinates in Riemann and Lobachevsky spaces, naturally related with Euler angle-parameters. Conclusion may be drawn: the general method of separation of variables embraces the all plane wave solutions; the plane waves in Lobachevsky and Riemann space consist of a small part of the whole set of basis wave functions of Schrödinger equation. In space of constant positive curvature $S_3$, a complex analog of horospherical coordinates of Lobachevsky space $H_3$ is introduced. To parameterize real space $S_3$, two complex coordinates $(r,z)$ must obey additional restriction in the form of the equation $r^2=e^{z-z^{\ast }}-e^{2z}$. The metrical tensor of space $S_3$ is expressed in terms of $(r,z)$ with additional constraint, or through pairs of conjugate variables $(r,r^{\ast })$ or $(z,z^{\ast })$; correspondingly exist three different representations for Schrödinger Hamiltonian. Shapiro plane waves are determined and explored as solutions of Schrödinger equation in complex horosperical coordinates of $S_3$. In particular, two oppositely directed plane waves may be presented as exponentials in conjugated coordinates. ${\Psi }_{-}=e^{-\alpha z}$ and ${\Psi }_{+}=e^{-\alpha z^{\ast }}$. Solutions constructed are single-valued, finite, and continuous functions in spherical space and correspond to discrete energy levels.

19 pages

References in corpus (1)

• The Runge-Lenz vector for quantum Kepler problem in the space of positive constant curvature and complex parabolic coordinates

Cited by in corpus (1)

• Quasi-plane waves for a particle with spin 1/2 on the background of Lobachevsky geometry: simulating of a special medium