Coupling the thermal scalar to the gravi-dilaton action shows winding modes can oppose or reverse expansion below the Hagedorn temperature, enable Brustein-Veneziano branch changes above it without graceful exit, and that the quadratic theory breaks down at the transition itself.
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Cosmological Dynamics of the Thermal Scalar Near the Hagedorn Temperature
Coupling the thermal scalar to the gravi-dilaton action shows winding modes can oppose or reverse expansion below the Hagedorn temperature, enable Brustein-Veneziano branch changes above it without graceful exit, and that the quadratic theory breaks down at the transition itself.