Black Holes and Quantum Mechanics
| dc.creator | Kallosh, Renata | |
| dc.date | 1999-01-31 | |
| dc.date.accessioned | 2026-07-07T04:25:55Z | |
| dc.date.available | 2026-07-07T04:25:55Z | |
| dc.description | The motion of a particle near the RN black hole horizon is described by conformal mechanics. Models of this type have no ground state with vanishing energy. This problem was resolved in past by a redefinition of the Hamiltonian which breaks translational time invariance but gives a normalizable ground state. We show that this change of the Hamiltonian is a quantum mechanical equivalent of the change of coordinates near the black hole horizon removing the singularity. The new Hamiltonian of quantum mechanics is identified as an operator of a rotation between 2 time-like coordinates of the adS hypersurface which translates global time. Therefore conformal quantum mechanics may eventually help to resolve the puzzles of the classical black hole physics. | |
| dc.description | 7 pages, Latex. To be published in proceedings of the 22nd Johns Hopkins Workshop, Gothenburg, 1998 | |
| dc.identifier | https://arxiv.org/abs/hep-th/9902007 | |
| dc.identifier | http://arxiv.org/abs/hep-th/9902007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/55919 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Black Holes and Quantum Mechanics | |
| dc.type | text |