Accelerating universe as a result of an adjustment mechanism
Prado Martin-Moruno, Nelson J. Nunes

TL;DR
This paper proposes a scalar-tensor gravity model with a de Sitter vacuum that can dynamically screen vacuum energy, leading to cosmological evolutions consistent with an accelerating universe.
Contribution
It introduces a class of scalar-tensor models with second order equations that maintain a de Sitter critical point regardless of matter content, offering a new approach to cosmic acceleration.
Findings
Models exhibit stable de Sitter solutions for various matter contents
Potential to explain universe's acceleration without fine-tuning vacuum energy
Framework compatible with general scalar-tensor theories
Abstract
In this essay we propose that the theory of gravity's vacuum is described by a de Sitter geometry. Under this assumption we consider an adjustment mechanism able to screen any value of the vacuum energy of the matter fields. We discuss the most general scalar-tensor cosmological models with second order equations of motion that have a fixed de Sitter critical point for any kind of material content. These models give rise to interesting cosmological evolutions that we shall discuss.
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