Simple (SISYPHUS) dynamical model of the cosmological constant
Vladan Pankovic

TL;DR
This paper proposes a simple dynamical model for the cosmological constant using a scalar field and Lagrangian formalism, aligning with observational data and illustrating a Sisyphus-like scalar field evolution.
Contribution
It introduces a novel scalar field-based dynamical model of dark energy, with exact solutions and a potential energy density featuring a maximum, inspired by chaotic inflation.
Findings
Model aligns with recent astronomical observations.
Scalar field tends to a final value exponentially.
Potential energy density has a unique maximum.
Abstract
In this work we suggest (in a formal analogy with Linde chaotic inflation scenario) simple dynamical model of the dark energy or cosmological constant. Concretely, we suggest a Lagrangian dependent of Universe scale factor and scalar field (with constant and positive total energy density as cosmological constant). Then, Euler-Lagrange equation for Universe scale factor is equivalent to the second Friedman equation for the flat empty space with cosmological constant (in this sense our model is full agreement with recent astronomical observations). Also there is Euler-Lagrange equation for scalar field that includes additional "friction" term and negative first partial derivative of unknown potential energy density (this equation is, in some way, similar to Klein-Gordon equation modified for cosmic expansion in Linde chaotic inflation scenario). Finally, total time derivative of the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Relativity and Gravitational Theory
