1998
DOI: 10.4310/atmp.1998.v2.n2.a1
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The large $N$ limit of superconformal field theories and supergravity

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Cited by 15,251 publications
(20,922 citation statements)
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References 47 publications
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“…Nevertheless, the construction of dS vacua has been achieved by taking into account a small number of D 3 -branes along with the AdS vacua in a type IIB string theory [3]. On the other hand, anti de Sitter (AdS) spaces are well understood in a string theory due its established correspondence with the gauge theory at its boundary [4,5].…”
Section: Introductionmentioning
confidence: 99%
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“…Nevertheless, the construction of dS vacua has been achieved by taking into account a small number of D 3 -branes along with the AdS vacua in a type IIB string theory [3]. On the other hand, anti de Sitter (AdS) spaces are well understood in a string theory due its established correspondence with the gauge theory at its boundary [4,5].…”
Section: Introductionmentioning
confidence: 99%
“…In particular, we revisit a curved brane-world [13] underlying a noncommutative U (1) gauge theory on a D 3 -brane [22]. We obtain generalized dS 4 and AdS 4 geometries leading to an axially symmetric and a spherically symmetric black holes.…”
Section: Introductionmentioning
confidence: 99%
“…In this Section, we will extend this analogy to the FRW equations under consideration. Let us first investigate this analogy in Einstein gravity for the usual (n + 1)-dimensional FRW Universe with a metric 1) where the n-dimensional spatial hypersurfaces with negative, zero or positive curvature are parametrized by k = −1, 0, 1, respectively 6 . We limit our discussion mainly to that of the closed universe (k = 1), with a spatial volume defined by V = a n d n x √ g. The standard FRW equations may then be written as 2) where …”
Section: Cosmological Entropy and Generalized Cardy-verlinde Formulamentioning
confidence: 99%
“…The action is given by 1 1) where c is an arbitrary coupling constant, κ 2 parametrizes the (d + 1)-dimensional Planck mass, the Riemann tensor, R µνξσ , and its contractions are constructed from the metric, g µν , and its derivatives, g ≡ detg µν and Λ represents the bulk cosmological constant. By extremising the variations of the action (2.1) with respect to the metric tensor and gauge field, respectively, we obtain the field equations…”
Section: Bulk Black Hole Geometry and Brane Dynamicsmentioning
confidence: 99%
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