1996/02/21 by Curtis G. Callan, Juan M. Maldacena · 3 citations
Physics and Astronomy · #hep-th
paper · pdf · doi:10.1016/0550-3213(96)00225-8
published as Nucl.Phys.B472:591-610,1996 · 18 pages, uses harvmac and psfig. The new version of the paper corrects various errors, omissions and obscurities of the original submission. The major error was an underestimate of the severity of the strong coupling problem in the D-brane description of black holes with a macroscopic event horizon. The new version has a more sober, but still optimistic assessment of what aspects of black hole quantum mechanics are be brought under control by D-branes. We thank several correspondents for helpful criticism and advice
arxiv created 1996/02/21 · arxiv updated 2011/05/05
Strominger and Vafa have used D-brane technology to identify and precisely count the degenerate quantum states responsible for the entropy of certain extremal, BPS-saturated black holes. Here we give a Type-II D-brane description of a class of extremal \it and non-extremal five-dimensional Reissner-Nordström solutions and identify a corresponding set of degenerate D-brane configurations. We use this information to do a string theory calculation of the entropy, radiation rate and ``Hawking'' temperature. The results agree perfectly with standard Hawking results for the corresponding nearly extremal Reissner-Nordström black holes. Although these calculations suffer from open-string strong coupling problems, we give some reasons to believe that they are nonetheless qualitatively reliable. In this optimistic scenario there would be no ``information loss'' in black hole quantum evolution.