The Conformal Version of Black Hole Thermodynamics
| dc.creator | Wu, Shuang-Qing | |
| dc.date | 2004-10-30 | |
| dc.date | 2004-12-29 | |
| dc.date.accessioned | 2026-07-07T04:17:42Z | |
| dc.date.available | 2026-07-07T04:17:42Z | |
| dc.description | The conformal thermodynamics of rotating charged black holes in general relativity and string theory is proposed by considering the first laws of thermodynamics for a pair of systems made up of the two horizons of a Kerr-Newman or Kerr-Sen black hole. These two systems are constructed by only demanding their ``horizon areas'' to be the sum and difference of that of the outer and inner horizons of their prototype. The thermodynamics present here is a ``conformal version'' of black hole thermodynamics, since it is closely related to the near-horizon conformal symmetry of black holes. The concept of non-quasinormal modes recently proposed by D. Birmingham and S. Carlip [9] is compatible with this ``conformal thermodynamics'', rather than the usual ``horizon thermodynamics''. In addition, we show that this conformal thermodynamics resembles to the thermodynamics of effective string or D-brane models, since the two newly-constructed systems bear a striking resemblance to the right- and left-movers in string theory and D-brane physics. | |
| dc.description | 6 pages, Revtex 4. New references added and further revised version | |
| dc.identifier | https://arxiv.org/abs/hep-th/0411002 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0411002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/52867 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The Conformal Version of Black Hole Thermodynamics | |
| dc.type | text |