1997
DOI: 10.1016/s0370-2693(96)01460-8
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D-branes and spinning black holes

Abstract: We obtain a new class of spinning charged extremal black holes in five dimensions, considered both as classical configurations and in the Dirichlet(D)-brane representation. The degeneracy of states is computed from the D-brane side and the entropy agrees perfectly with that obtained from the black hole side. 2/96♣

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Cited by 580 publications
(1,068 citation statements)
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“…Step 1 The first equation to solve is the homogeneous one, (21), which implies that the G i satisfy the Euclidean, vacuum Maxwell equations. Conversely, given a solution, F , to the Maxwell equations one can take G i = F + * F .…”
Section: Finding Solutionsmentioning
confidence: 99%
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“…Step 1 The first equation to solve is the homogeneous one, (21), which implies that the G i satisfy the Euclidean, vacuum Maxwell equations. Conversely, given a solution, F , to the Maxwell equations one can take G i = F + * F .…”
Section: Finding Solutionsmentioning
confidence: 99%
“…(It is also surprising that the equations that govern the G i are completely independent of the metric coefficients A i !) For the solutions that we seek, the G i are sourced by the dipole M5 branes, and so the G i must fall off suitably fast at infinity, and the location and shape of these branes thus completely determines the solution to (21). Since there are three independent G i 's, there are three independent source distributions to be chosen.…”
Section: Finding Solutionsmentioning
confidence: 99%
See 1 more Smart Citation
“…These are the 5D spinning black holes [4], characterized by membrane charges q A and angular momentum J L associated to the U (1) L isometry. Their characteristic size r BH grows as the square root of the graviphoton charge √ Q which in turn is proportional to the membrane charge q A .…”
Section: → Iiamentioning
confidence: 99%
“…index) Z should not depend on the radius R, yielding an equality of the form Z 4D = Z 5D with a certain relation between the arguments. The microscopic description for many (but not all) 5D spinning black holes is known [3,4]. Hence this 5D-4D relation gives a microscopic description of 4D black holes for many cases in which it had previously been unknown.…”
Section: Introductionmentioning
confidence: 99%