Slinky evolution of domain wall brane cosmology
Avihay Kadosh, Aharon Davidson, Elisabetta Pallante

TL;DR
This paper introduces a novel brane cosmology model where the formation and evolution of the universe are driven by a symmetry breaking mechanism involving an initial symmetry between time and an extra spatial dimension, leading to a decaying cosmological constant.
Contribution
It proposes a new scenario with a symmetry-based formation of branes and cosmology, introducing slinky configurations with a decaying cosmological constant, and analyzes their physical viability.
Findings
Slinky configurations exhibit a decaying cosmological constant.
A simplified model with a constrained watershed is constructed.
Conditions for realistic cosmological evolution are discussed.
Abstract
Invoking an initial symmetry between the time and some extra spatial dimension , we discuss a novel scenario where the dynamical formation of the 4-dim brane and its cosmological evolution are induced simultaneously by a common symmetry breaking mechanism. The local maximum of the underlying scalar potential is mapped onto a 'watershed' curve in the plane; the direction tangent to this curve is identified as the cosmic time, whereas the perpendicular direction serves locally as the extra spatial dimension. Special attention is devoted to the so-called slinky configurations, whose brane cosmology is characterized by a decaying cosmological constant along the watershed curve. Such a slinky solution is first constructed within a simplified case where the watershed is constrained by . The physical requirements for a slinky configuration to generate a…
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