Higher Spin Resolution of a Toy Big Bang
  Diffeomorphisms preserve spacetime singularities, whereas higher spin
symmetries need not. Since three dimensional de Sitter space has quotients that
have big-bang/big-crunch singularities and since dS_3-gravity can be written as
an SL(2,C) Chern-Simons theory, we investigate SL(3,C) Chern-Simons theory as a
higher-spin context in which these singularities might get resolved. As in the
case of higher spin black holes in AdS_3, the solutions are invariantly
characterized by their holonomies. We show that the dS_3 quotient singularity
can be de-singularized by an SL(3,C) gauge transformation that preserves the
holonomy: this is a higher spin resolution the cosmological singularity. Our
work deals exclusively with the bulk theory, and is independent of the
subtleties involved in defining a CFT_2 dual to dS_3 in the sense of dS/CFT.
