Time Dependence

Tae Jun Park

We solve the Schrodinger equation analytically for systems whose potentials have a certain time-dependence (which is monotonously decreasing) and general coordinate-dependences.Only a few time-dependent systems have been reported to be analytically solved whose potentials are constant, linear, and quadratic functions of coordinate with arbitrary time-dependences.From a different perspective, we focus on the time-dependent systems whose potentials are monotonously decreasing functions of time with arbitrary coordinate dependences.Time-dependent potential of any coordinate-dependence can be handled analytically by transforming it to a time-independent potential of known solutions if its time-dependence is monotonously decreasing.We do this by a unitary transformation of the wavefunction and variable transformations to change the Schrodinger equation to be time-independent in new variables.These variables are then determined by solving a set of simple differential equations.This way we are able to find and to obtain analytical solutions for time-dependent potentials which we mention above.

Bu-Xing Xu, A. K. Rajagopal

It is proved that the mapping, time-dependent potential \ensuremath{\rightarrow} time-dependent density, is not invertible, in general, over the class of all potentials expandable in a Taylor series with respect to time coordinates. However, an invertible mapping does exist between the time-dependent potential and time-dependent current density. To explore this in detail, a one-body time-dependent problem is examined in an attempt to seek a time-dependent current-density-functional formalism.

P. R. Berman

Leonardo Angelini

Andreas Fring, M. H. Y. Moussa

It has been argued that it is incompatible to maintain unitary time evolution for time-dependent non-Hermitian Hamiltonians when the metric operator is explicitly time dependent. We demonstrate here that the time-dependent Dyson equation and the time-dependent quasi-Hermiticity relation can be solved consistently in such a scenario for a time-dependent Dyson map and time-dependent metric operator, respectively. These solutions are obtained at the cost of rendering the non-Hermitian Hamiltonian to be a nonobservable operator as it ceases to be quasi-Hermitian when the metric becomes time dependent.