3.00 pm, Seminar Hall Near horizon dynamics of three dimensional black holes Daniel Grumiller Institute for Theoretical Physics, TU Wien (Vienna University of Technology). 22-08-19 Abstract The Hamiltonian reduction of three dimensional Einstein gravity with negative cosmological constant under constraints imposed by near horizon boundary conditions yields a Floreanini-Jackiw type scalar field theory on the horizon. I discuss a derivation of this result and consequences, particularly for soft hair excitations on the horizon.
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