  We statistically study gamma-ray burst (GRB) optical flares from the
Swift/UVOT catalog. We compile 119 optical flares, including 77 flares with
redshift measurements. Some tight correlations among the time scales of optical
flares are found. For example, the rise time is correlated with the decay time,
and the duration time is correlated with the peak time of optical flares. These
two tight correlations indicate that longer rise times are associated with
longer decay times of optical flares, and also suggest that broader optical
flares peak at later times, which are consistent with the corresponding
correlations of X-ray flares. We also study the frequency distributions of
optical flare parameters, including the duration time, rise time, decay time,
peak time and waiting time. Similar power-law distributions for optical and
X-ray flares are found. Our statistic results imply that GRB optical flares and
X-ray flares may share the similar physical origin and both of them are
possibly related to central engine activities.
