arXiv · hep-th/0211212
Remarks on Black Hole Instabilities and Closed String Tachyons
Abstract
Physical arguments stemming from the theory of black-hole thermodynamics are used to put constraints on the dynamics of closed-string tachyon condensation in Scherk--Schwarz compactifications. A geometrical interpretation of the tachyon condensation involves an effective capping of a noncontractible cycle, thus removing the very topology that supports the tachyons. A semiclassical regime is identified in which the matching between the tachyon condensation and the black-hole instability flow is possible. We formulate a generalized correspondence principle and illustrate it in several different circumstances: an Euclidean interpretation of the transition from strings to black holes across the Hagedorn temperature and instabilities in the brane-antibrane system.
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J. L. F. Barbon, E. Rabinovici. 2002-11-22. Remarks on Black Hole Instabilities and Closed String Tachyons. https://doi.org/10.1023/a%3A1022823926674
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