The
space charge region (SCR) is a majority carrier-depleted region
in a semiconductor. The width of this region and the size of the potential
drop across it control photochemical charge separation under illumination,
as relevant to solar energy conversion with photocatalyst particles,
for example. For photocatalysts, the space charge region is often
difficult to evaluate due to the small dimensions of the particles.
Here, we show that surface photovoltage spectroscopy (SPS) can be
used to observe the SCR in nano- and microparticles of strontium titanate
(SrTiO3), aluminum-doped strontium titanate, and gallium
arsenide (GaAs) on gold substrates. Depending on particle film thickness
and thermal annealing conditions, we observe negative or positive
photovoltages corresponding to majority or minority carrier diffusion
toward the gold substrate. The direction of charge transport is controlled
by the potential barrier across the depletion layer at the gold-particle
interface. From the inverted photovoltage signal, potential barriers
are estimated between 0.005 and 0.189 V and SCR widths between 1.3
and 2.8 μm. The observed barriers are 10–100 times smaller
than the theory for an ideal Schottky junction, and the observed SCR
widths are up to 100 times larger. The difference can be attributed
to trapping of majority carriers in surface states arising from broken
bonds and disorder, in the case of GaAs, or from chemisorbed oxygen,
in the case of SrTiO3. Trapping of majority carriers in
surface states (Fermi level pinning) also diminishes the effective
carrier concentrations in the particles, explaining the larger SCR
width in the films. These findings showcase the importance of surface
states for charge separation in photocatalyst particles and their
films.