Analytic approximation to 5 dimensional Black Holes with one compact dimension
arXiv:hep-th/0410078 · doi:10.1103/PhysRevD.71.024024
Abstract
We study black hole solutions in space, using an expansion to fourth order in the ratio of the radius of the horizon, , and the circumference of the compact dimension, . A study of geometric and thermodynamic properties indicates that the black hole fills the space in the compact dimension at . At the same value of the entropies of the uniform black string and of the black hole are approximately equal.
21 pages, 4 figures. Replaces previous version, with added references and slightly altered discussion
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- The Phase Transition between Caged Black Holes and Black Strings - A Review
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- Non-Relativistic Gravitation: From Newton to Einstein and Back
- Classical Effective Field Theory and Caged Black Holes
- Towers of Gravitational Theories
- Thermal phases of D1-branes on a circle from lattice super Yang-Mills
- Thermodynamics of static black objects in D dimensional Einstein-Gauss-Bonnet gravity with D-4 compact dimensions
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- New stable phase of non-uniform charged black strings
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- The decay of hot KK space
- First Law of p-brane Thermodynamics
- Black Topologies Production in Extra Dimensions
- Entropy of Three-Charge Black Holes on a Circle