Holographic formulation of quantum supergravity

We show that $\mathcal{N}=1\mathrm{}$ supergravity with a cosmological constant can be expressed as constrained topological field theory based on the supergroup $Osp\left(1\mathrm{}|4\right).$ The theory is then extended to include timelike boundaries with finite spatial area. Consistent boundary conditions are found which induce a boundary theory based on a supersymmetric Chern-Simons theory. The boundary state space is constructed from states of the boundary supersymmetric Chern-Simons theory on the punctured two sphere and naturally satisfies the Bekenstein bound, where area is measured by the area operator of quantum supergravity.