Non-Hermitian Swanson model with a time-dependent metric

Andreas Fring and Miled H. Y. Moussa
Phys. Rev. A 94, 042128 – Published 26 October 2016

Abstract

We provide further nontrivial solutions to the recently proposed time-dependent Dyson and quasi-Hermiticity relation. Here, we solve them for the generalized version of the non-Hermitian Swanson Hamiltonian with time-dependent coefficients. We construct time-dependent solutions by employing the Lewis-Riesenfeld method of invariants and discuss concrete physical applications of our results.

  • Received 22 June 2016

DOI:https://doi.org/10.1103/PhysRevA.94.042128

©2016 American Physical Society

Physics Subject Headings (PhySH)

General Physics

Authors & Affiliations

Andreas Fring1 and Miled H. Y. Moussa1,2

  • 1Department of Mathematics, City University London, Northampton Square, London EC1V 0HB, United Kingdom
  • 2Instituto de Física de São Carlos, Universidade de São Paulo, P.O. Box 369, São Carlos, 13560-970, São Paulo, Brazil

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Issue

Vol. 94, Iss. 4 — October 2016

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