2017
DOI: 10.1140/epjp/i2017-11524-7
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On the invariant method for the time-dependent non-Hermitian Hamiltonians

Abstract: We propose a scheme to deal with certain time-dependent non-Hermitian Hamiltonian operators H(t) that generate a real phase in their time-evolution. This involves the use of invariant operators I P H (t) that are pseudo-Hermitian with respect to the time-dependent metric operator, which implies that the dynamics is governed by unitary time evolution. Furthermore, H(t) is generally not quasi-Hermitian and does not define an observable of the system but I P H (t) obeys a quasi-hermiticity transformation as in th… Show more

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Cited by 54 publications
(39 citation statements)
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References 28 publications
(46 reference statements)
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“…As for Lewis-Riesenfeld invariants for Non-Hermitian Hamiltonians, they can be generalized in two different forms (Simón et al, 2018) corresponding to (Gao et al, 1992;Khantoul et al, 2017;)…”
Section: Non-hermitian Hamiltoniansmentioning
confidence: 99%
“…As for Lewis-Riesenfeld invariants for Non-Hermitian Hamiltonians, they can be generalized in two different forms (Simón et al, 2018) corresponding to (Gao et al, 1992;Khantoul et al, 2017;)…”
Section: Non-hermitian Hamiltoniansmentioning
confidence: 99%
“…It is precisely this omission that we aim to remedy here. This technical complexity also probably explains why only a relatively few realistic applications of several alternative implementations of the NHIP ideas themselves may yet be found in the current literature [30,[72][73][74][75][76][77][78][79][80][81].…”
Section: B the Physical Hilbert Space Metric Operatormentioning
confidence: 99%
“…The most efficient way to solve the time-dependent Dyson equation (1.3) is to use the Lewis-Riesenfeld approach [27] and compute at first the respective time-dependent invariants I h (t) and I H (t) for the Hamiltonian h(t) and H(t), see [28,29,22], by solving the equations…”
Section: Quasi-exactly Solvable Lewis-riesenfeld Invariantsmentioning
confidence: 99%