Quintessence and effective RN de Sitter brane geometries
K. Priyabrat Pandey, Abhishek K. Singh, Sunita Singh, Richa Kapoor and, Supriya Kar

TL;DR
This paper explores how non-linear gauge dynamics and torsion in string theory can lead to emergent de Sitter universes, quantum black holes, and potential explanations for dark energy and cosmic acceleration.
Contribution
It introduces a novel framework linking torsion, gauge dynamics, and brane configurations to emergent cosmological phenomena and black hole solutions in string theory.
Findings
Emergence of de Sitter universe from brane pair creation
Existence of non-singular quantum black holes with torsion
Potential source of dark energy from axion on anti-brane
Abstract
We revisit an effective space-time torsion curvature in a second order formalism, underlying the non-linear gauge dynamics, of a two form on a -brane in type IIA superstring theory. The formalism incorporates the significance of a global NS two form into the theory via its perturbative coupling to a dynamical two form. In particular, we explore the non-linear gauge dynamics on a -brane in presence of a non-trivial background metric. The fact that the global modes of a NS two form in an open string theory sources the background metric on a -brane may hint at the existence of an anti -brane in the formalism. An effective de Sitter universe is shown to emerge on a vacuum created pair of -brane by a local two form at the past horizon with a Big Bang. We obtain a number of 4D de Sitter quantum black holes, including a Reissner-Nordstrom vacuum, with…
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