Non-BPS black holes and self-interacting fundamental strings

Abstract

The string-black hole correspondence principle can be investigated in the non-BPS scenario by studying the string configuration and entropy when the string coupling is slowly increased. Through a rigorous analysis, it is shown how an ensemble of string states at fixed mass and Neveu-Schwarz charges gets dominated in any dimension by compact states for which the one-loop corrections are important (possibly signaling the transition to a black hole regime/description) and with a size (spread) within the horizon radius of the expected correspondent black holes.

Comments: Proceedings of the Twelfth Marcel Grossmann Meeting on General Relativity, Paris, France, 12-18 july 2009.