On the thermodynamic instability of LST
arXiv:hep-th/0107102
Abstract
The high energy thermodynamics of Little String Theory (LST) is known to be unstable. An unresolved question is whether the corresponding instability in LST holographic dual is of stringy or supergravity origin. We study UV thermodynamics of a large metric deformation of the LST dual realized (in the extremal case) by type IIB fivebranes wrapping a two-sphere of a resolved conifold, and demonstrate that the resulting black hole has negative specific heat. This explicitly shows that the high energy thermodynamic instability of the LST holographic dual is of the supergravity origin.
14 pages, 1 figure, v2: reference added
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- Black Holes on Cylinders
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- A holographic perspective on Gubser-Mitra conjecture
- Holography and Unquenched Quark-Gluon Plasmas
- The Silence of the Little Strings
- Thermal Correlators in Little String Theory
- Thermodynamics of the Near-Extremal NS5-brane
- Hagedorn Systems from Backreacted Finite Temperature N_f=2N_c Backgrounds
- 5d Black holes, wrapped fivebranes and 3d Chern-Simons Super Yang-Mills
- Hagedorn String Thermodynamics in Curved Spacetimes and near Black Hole Horizons
- On Non-Critical Superstring/Black Hole Transition