Geometric actions and flat space holography
arXiv:1912.08207 · doi:10.1007/JHEP02(2020)125
Abstract
In this paper we perform the Hamiltonian reduction of the action for three-dimensional Einstein gravity with vanishing cosmological constant using the Chern-Simons formulation and Bondi-van der Burg-Metzner-Sachs (BMS) boundary conditions. An equivalent formulation of the boundary action is the geometric action on BMS coadjoint orbits, where the orbit representative is identified as the bulk holonomy. We use this reduced action to compute one-loop contributions to the torus partition function of all BMS descendants of Minkowski spacetime and cosmological solutions in flat space. We then consider Wilson lines in the ISO Chern-Simons theory with endpoints on the boundary, whose reduction to the boundary theory gives a bilocal operator. We use the expectation values and two-point correlation functions of these bilocal operators to compute quantum contributions to the entanglement entropy of a single interval for BMS invariant field theories and BMS blocks, respectively. While semi-classically the BMS boundary theory has central charges and , we find that quantum corrections in flat space do not renormalize , but rather lead to a non-zero .
arXiv comment61 pages, v2: typo's fixed and ref's added, v3: added comments and improved discussions. Matches version accepted for publication in JHEP
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