Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 18, Issue 10, Pages 1823-1834Publisher
IOP Publishing Ltd
DOI: 10.1088/0264-9381/18/10/301
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It is argued that the diffeomorphism on the horizontal sphere can be regarded as a non-trivial asymptotic isometry of the Schwarzschild black hole. We propose a new boundary condition of asymptotic metrics near the horizon and show that the condition admits the local time shift and diffeomorphism on the horizon as the asymptotic symmetry.
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