Abstract
We derive an exact expression for the photocurrent of photo-emission spectroscopy using time-dependent current density functional theory (TDCDFT). This expression is given as an integral over the Kohn-Sham spectral function renormalized by effective potentials that depend on the exchange-correlation kernel of current density functional theory. We analyze in detail the physical content of this expression by making a connection between the density-functional expression and the diagrammatic expansion of the photocurrent within many-body perturbation theory. We further demonstrate that the density functional expression does not provide us with information on the kinetic energy distribution of the photo-electrons. Such information can, in principle, be obtained from TDCDFT by exactly modeling the experiment in which the photocurrent is split into energy contributions by means of an external electromagnetic field outside the sample, as is done in standard detectors. We find, however, that this procedure produces very nonlocal correlations between the exchange-correlation fields in the sample and the detector.
Highlights
We derived an exact expression within time-dependent current-density functional theory (TDCDFT) for the photocurrent of photo-emission spectroscopy
This expression involves an integral over the Kohn-Sham spectral function weighted with effective Kohn-Sham one-body interactions
This expression directly gives the angular dependence of the photocurrent it does not provide us directly with the kinetic energy distribution of the photo-electrons
Summary
In TDCDFT, this current density is calculated instead from a Kohn-Sham state | s(t) with a time-evolution determined by a non-interacting Kohn-Sham Hamiltonian Hs(t). This Hamiltonian contains an external Kohn-Sham vector field As (in a gauge where we absorb the scalar potentials in a vector potential) which is a functional of the current density. In this way, the photo-emission experiment can be modelled theoretically by time-propagation of Kohn-Sham orbitals after a suitable approximation for the Kohn-Sham vector potential As has been chosen.
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