Demonstrates vacuum selection mechanisms in dark energy models, implying new insights.
This paper introduces a dynamical mechanism for vacuum selectionbased on a relaxation equation for dark energy density. We demonstrate that the system develops a critical surfacewhere the effective description breaks down, naturally drivingthe evolution toward a de Sitter attractor. The mechanism does not rely on fine-tuning and follows fromthe structure of the dynamical system.
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Alik Gimranov (2026) studied this question.
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