Abstract

A geometric torsion dynamics leading to an effective curvature in a second order formalism on a D4-brane is revisited with a renewed interest. We obtain two effective AdS4AdS_4 brane geometries on a vacuum created pair of (DDˉ)3(D{\bar D})_3-brane. One of them is shown to describe an AdS Schwarzschild spinning black hole and the other is shown to describe a spinning black hole bound state. It is argued that a D-instanton in a vacuum created anti D3-brane within a pair may describe a quintessence. It may seen to incorporate a varying vacuum energy density in a brane universe. We consider the effective curvature scalar on S1×S1S^1\times S^1 to analyze torsion-less geometries on a vacuum created pair of (DDˉ)2(D{\bar D})_2-brane. The emergent AdS3AdS_3 brane is shown to describe a Schwarzschild and a Reissner-Nordstrom (RN) geometries in presence of extra dimension(s).

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