A note on the string spectrum at the Hagedorn temperature

Details A note on the string spectrum at the Hagedorn temperature A note on the string spectrum at the Hagedorn temperature

2009-05-21

arxiv.org/abs/0905.3578v1

Physics

High Energy Physics

High Energy Physics - Theory

Latex 19 pages

Scientific paper

We discuss semi-classical string configurations at finite temperature. We find that those soliton solution in the background describing type IIA strings disappear or become divergent when we approach the Hagedorn temperature in the strong coupling regime. These findings together with a semi-classical analysis for the Hawking radiation let us to think that Hawking radiation is mainly driven by the existence of highly excited states. As by side, we check that beside the thermodynamical instability the system is dynamical unstable before reaching the Hagedorn temperature.

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