Size of Black Holes through Polymer Scaling
S. Kalyana Rama

TL;DR
This paper models black hole horizons as polymer-like strings, using scaling laws to determine their size and explaining the transition between black hole and string states, including extremal cases.
Contribution
It introduces a polymer-based model for black hole horizons and derives their size through scaling laws, providing a new perspective on black hole-string transitions.
Findings
Derived black hole size using polymer scaling laws
Explained black hole to string state transition
Extended explanation to extremal black holes
Abstract
We imagine the strings on the stretched horizon of any 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.
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