Size of Black Holes through Polymer Scaling

Abstract

We imagine the strings on the stretched horizon of any $d$ space-time dimensional black hole to be bits of polymer. Then, proposing an interaction between these bits we obtain the size of the configuration, and thus of the black hole, using the scaling laws. The transition from a typical black hole state to a typical string state has a simple explanation, which also holds for the extremal black holes.

Latex file, 8 pages

References in corpus (3)

• Microscopic Origin of the Bekenstein-Hawking Entropy
• M Theory As A Matrix Model: A Conjecture
• A Correspondence Principle for Black Holes and Strings

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• A Description of Schwarzschild Black Holes in terms of Intersecting M-branes and antibranes
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• Role of Chaplygin gas as geometrical dark energy in anisotropic brane gravity
• Size scaling of self gravitating polymers and strings