We
present an accurate approach to compute X-ray photoelectron
spectra based on the GW Green’s function method
that overcomes the shortcomings of common density functional theory
approaches. GW has become a popular tool to compute
valence excitations for a wide range of materials. However, core-level
spectroscopy is thus far almost uncharted in GW.
We show that single-shot perturbation calculations in the G0W0 approximation,
which are routinely used for valence states, cannot be applied for
core levels and suffer from an extreme, erroneous transfer of spectral
weight to the satellite spectrum. The correct behavior can be restored
by partial self-consistent GW schemes or by using
hybrid functionals with almost 50% of exact exchange as a starting
point for G0W0. We also include relativistic corrections and present a benchmark
study for 65 molecular 1s excitations. Our absolute and relative GW core-level binding energies agree within 0.3 and 0.2
eV with experiment, respectively