Classical and Semiclassical Stability of Emergent Universes in Jordan-Brans-Dicke Theory
Pedro Labra\~na, Juan Ortiz

TL;DR
This paper examines the stability of emergent universe models in Jordan-Brans-Dicke theory, demonstrating that with appropriate parameters, these models can be stable against classical and certain semiclassical tunneling instabilities.
Contribution
It provides a detailed analysis of classical and semiclassical stability of Einstein static states in Jordan-Brans-Dicke theory, identifying conditions for robustness against quantum decay.
Findings
ES configuration can be stable with suitable JBD potential and parameters.
Quantum tunneling instability can be avoided in certain parameter regions.
Some tunneling processes remain possible beyond the analyzed scope.
Abstract
The Emergent Universe scenario is based on the assumption that the universe originates from a past-eternal Einstein static (ES) state, subsequently evolving toward an inflationary phase and a hot Big Bang era. Such models are appealing as they provide nonsingular and geodesically complete cosmological histories. However, it has been argued by Mithani and Vilenkin that, even when the ES state is classically stable, certain models can admit semiclassical tunneling channels leading to quantum decay toward configurations of vanishing scale factor. In this work, we investigate the classical and semiclassical stability of the ES regime in the context of Jordan-Brans-Dicke (JBD) theory. We analyze the structure of the Wheeler-DeWitt potential in minisuperspace and study representative semiclassical tunneling channels compatible with the Hamiltonian constraint. We show that, for suitable…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
