Near horizon dynamics of three dimensional black holes
Keyword(s):
We perform the Hamiltonian reduction of three dimensional Einstein gravity with negative cosmological constant under constraints imposed by near horizon boundary conditions. The theory reduces to a Floreanini–Jackiw type scalar field theory on the horizon, where the scalar zero modes capture the global black hole charges. The near horizon Hamiltonian is a total derivative term, which explains the softness of all oscillator modes of the scalar field. We find also a (Korteweg–de Vries) hierarchy of modified boundary conditions that we use to lift the degeneracy of the soft hair excitations on the horizon.
1997 ◽
Vol 495
(3)
◽
pp. 477-504
◽
1995 ◽
Vol 10
(31)
◽
pp. 2367-2379
◽
Keyword(s):
2013 ◽
Vol 867
(2)
◽
pp. 483-505
◽
2015 ◽
Vol 30
(36)
◽
pp. 1550220
◽
Keyword(s):
2017 ◽
Vol 34
(18)
◽
pp. 184001
◽
Keyword(s):
Keyword(s):