Stable Emergent Universe -- A Creation without Big-Bang
Eduardo Guendelman, Ramon Herrera, Pedro Labrana, Emil Nissimov,, Svetlana Pacheva

TL;DR
This paper introduces a generalized gravity-matter model with two non-Riemannian volume forms, leading to an effective theory that unifies early universe inflation and dark energy, featuring a non-singular emergent universe solution.
Contribution
It develops a new class of gravity-matter models with two volume forms, resulting in an effective potential with two flat regions and a stable emergent universe solution.
Findings
Effective potential with two flat regions for inflation and dark energy
Existence of a non-singular stable emergent universe solution
Unified description of early universe and current accelerated expansion
Abstract
Based on an earlier introduced new class of generalized gravity-matter models defined in terms of two independent non-Riemannian volume forms (alternative generally covariant integration measure densities) on the space-time manifold, we derive an effective "Einstein-frame" theory featuring the following remarkable properties: (i) We obtain effective potential for the cosmological scalar field possessing two infinitely large flat regions which allows for a unified description of both early universe inflation as well as of present dark energy epoch; (ii) For a specific parameter range the model possesses a non-singular stable "emergent universe" solution which describes an initial phase of evolution that precedes the inflationary phase.
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