  We have surveyed all 22 known Galactic globular clusters observable with the
Arecibo radio telescope and within 70kpc of the Sun for radio pulsations at
~1.4GHz. Data were taken with the Wideband Arecibo Pulsar Processor, which
provided the large bandwidth and high time and frequency resolution needed to
detect fast-spinning, faint pulsars. We have also employed advanced search
techniques to maintain sensitivity to short orbital period binaries. These
searches have discovered 11 new millisecond pulsars and 2 promising candidates
in 5 clusters, almost doubling the population of pulsars in the Arecibo-visible
globular clusters. Ten of these new pulsars are in binary systems, and 3 are
eclipsing. This survey has discovered significantly more very fast-spinning
pulsars (P_spin <~ 4ms) and short orbital period systems (P_orb <~ 6hr) than
previous surveys of the same clusters. We discuss some properties of these
systems, as well as some characteristics of the globular cluster pulsar
population in general, particularly its luminosity distribution.
