D. Gall et al., Electronic structure of ScN determined using optical spectroscopy, photoemission, and ab initio calculations - art. no. 125119, PHYS REV B, 6312(12), 2001, pp. 5119
Experimental and ab initio computational methods are employed to conclusive
ly show that ScN is a semiconductor rather than a semimetal, i.e., there is
a gap between the N 2p and the Sc 3d bands. Previous experimental investig
ators reported, in agreement with band structure calculations showing a ban
d overlap of 0.2 eV, that ScN is a semimetal while others concluded that it
is a semiconductor with a band gap larger than 2 eV. We have grown high qu
ality, single crystalline ScN layers on MgO(001) and on TiN(001) buffer lay
ers on MgO(001) by ultrahigh vacuum reactive magnetron sputter deposition.
ScN optical properties were determined by transmission, reflection, and spe
ctroscopic ellipsometry while in-situ x-ray and ultraviolet valence band ph
otoelectron spectroscopy were used to determine the density of stares (DOS)
below the Fermi level. The measured DOS exhibits peaks at 3.8 and 5.2 eV s
temming from the N 2p bands and at 15.3 eV due to the N 2s bands. The imagi
nary part of the measured dielectric function epsilon (2) consists of two p
rimary features due to direct X- and Gamma -point transitions at photon ene
rgies of 2.7 and 3.8 eV, respectively. For comparison, the ScN band structu
re was calculated using an nb initio Kohn-Sham approach which treats the ex
change interactions exactly within density-functional theory. Calculated DO
S and the complex dielectric function are in good agreement with our ScN va
lence-band photoelectron spectra and measured optical properties. respectiv
ely. We conclude, combining experimental and computational results, that Sc
N is a semiconductor with an indirect Gamma -X bandgap of 1.3 +/- 0.3 eV an
d a direct X-point gap of 2.4 +/- 0.3 eV.