Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 1823-1834 |
| Number of pages | 12 |
| Journal | Classical and Quantum Gravity |
| Volume | 18 |
| Issue number | 10 |
| DOIs | |
| Publication status | Published - 2001 May 21 |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)