Dynamical and static solutions to $R=0$-scalar-tensor theory
  We consider the most cosmologically interesting and relevant case of
scalar-tensor theory (STT) and derive new normal and phantom, dynamical and
static, solutions. We determine the Bianchi I Kasner exponents and show that
the dynamical solutions are heteroclinic orbits connecting two singularities.
Approaching the singularities, a purely transverse expansion (no radial
expansion or collapse) may occur.
