Statistical Entropy of Nonextremal Four-Dimensional Black Holes and U-Duality
G.T. Horowitz, D.A. Lowe, J.M. Maldacena

TL;DR
This paper explores the microscopic states in string theory responsible for the entropy of near-extremal and non-extremal rotating four-dimensional black holes, emphasizing duality invariance and entropy matching.
Contribution
It identifies the string theory states responsible for black hole entropy and extends entropy formulas to non-extremal, non-rotating black holes using duality invariance.
Findings
Exact match of Bekenstein-Hawking entropy for non-extremal black holes
Extension of near-extremal entropy formulas to far-from-extremal cases
Duality invariant formulation of black hole entropy
Abstract
We identify the states in string theory which are responsible for the entropy of near-extremal rotating four-dimensional black holes in supergravity. For black holes far from extremality (with no rotation), the Bekenstein-Hawking entropy is exactly matched by a mysterious duality invariant extension of the formulas derived for near-extremal black holes states.
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