  Exact, non-singular, time-dependent solutions of Maxwell-Einstein gravity
with and without dilatons are constructed by double Wick rotating a variety of
static, axisymmetric solutions. This procedure transforms arrays of charged or
neutral black holes into s-brane (spacelike brane) solutions, i.e. extended,
short-lived spacelike defects. Along the way, new static solutions
corresponding to arrays of alternating-charge Reissner-Nordstrom black holes,
as well as their dilatonic generalizations, are found. Their double Wick
rotation yields s-brane solutions which are periodic in imaginary time and
potential large-N duals for the creation/decay of unstable D-branes in string
theory.
