Abstract
I briefly review an emergent gravity scenario underlying a stringy pair production of brane/anti-brane universe by a KR field quanta on a \(D_4\)- barne. We obtain a generic family of ’quantum’ degenerate black holes in the emergent gravity underlying a dynamical Neveu-Schwarz (NS) field on a vacuum created stringy pair of a \((3{\bar{3}})\)-brane. In a low energy (GTR) limit the degeneracy disappear and the reduced vauca describe the Kerr family of macroscopic black holes in 4D.
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