The perpendicular-to-parallel size ratio of highly excited rotating strings agrees with rotating black holes at small angular momentum, with a random-walk model reproducing the sizes at all spins.
Asymptotic level density in heterotic string theory and rotating black holes
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abstract
We calculate the density of states with given mass and spin in string theory and obtain asymptotic formulas. We also compute the tree-level gyromagnetic couplings for arbitrary physical states in the heterotic string theory. These results are then applied to study whether fundamental strings can consistently describe the microphysics of the black hole horizon in the case of a general classical solution characterized by mass, charge and angular momentum.
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Size and Shape of Rotating Strings and the Correspondence to Black Holes
The perpendicular-to-parallel size ratio of highly excited rotating strings agrees with rotating black holes at small angular momentum, with a random-walk model reproducing the sizes at all spins.