Holographic Formulation of Quantum Supergravity
arXiv:hep-th/0009018 · doi:10.1103/PhysRevD.63.064010
Abstract
We show that supergravity with a cosmological constant can be expressed as constrained topological field theory based on the supergroup . 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.
30 pages, no figure
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Cited by in corpus (24)
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