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.
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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.