D-brane Approach to Black Hole Quantum Mechanics
Abstract
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-Nordstr\"om 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-Nordstr\"om 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.
Cite
@article{arxiv.hep-th/9602043,
title = {D-brane Approach to Black Hole Quantum Mechanics},
author = {Curtis G. Callan and Juan M. Maldacena},
journal= {arXiv preprint arXiv:hep-th/9602043},
year = {2011}
}
Comments
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