Relativistic full-potential photoemission theory is a straightforward gener
alization of the original well-established one-step model. This, so far, mo
st elaborated version of the theory has been applied to photocurrent calcul
ations for the GaAs(110) surface. Here we present angle-resolved ultraviole
t photoemission intensities calculated in normal emission for a range of di
fferent excitation energies. The investigation is based on a space-filling
cell potential, which has been determined self-consistently from a relativi
stic full-potential KKR bandstructure calculation. We compare our calculate
d photoemission spectra with muffin-tin results as well as with correspondi
ng experimental data. From this analysis we obtain an improved agreement be
tween experiment and theory, especially in the relative intensities occurri
ng in the different photoemission spectra. (C) 1999 Elsevier Science B.V. A
ll rights reserved.