Dark Energy as a Relic of the Vacuum-Energy Cancellation?
O. M. Lecian, G. Montani

TL;DR
This paper explores a modified gravity model with an exponential Lagrangian, proposing that dark energy may originate from vacuum-energy cancellation, and analyzes its implications for cosmic acceleration and deSitter solutions.
Contribution
It introduces a new exponential Lagrangian for gravity, linking dark energy to vacuum-energy cancellation and providing a scalar-tensor framework analysis.
Findings
DeSitter solutions exist only with negative vacuum-energy ratio.
Negative cosmological constant can induce accelerated deSitter expansion.
The model predicts non-Einsteinian effects in quantum regimes.
Abstract
We analyze the dynamical implications of an exponential Lagrangian density for the gravitational field, as referred to an isotropic FRW Universe. Then, we discuss the features of the generalized deSitter phase, predicted by the new Friedmann equation. The existence of a consistent deSitter solution arises only if the ratio between the vacuum-energy density and that associated with the fundamental length of the theory acquires a tantalizing negative character. This choice allows us to explain the present universe dark energy as a relic of the vacuum-energy cancellation due to the cosmological constant intrinsically contained in our scheme. The corresponding scalar-tensor description of the model is addressed too, and the behavior of the scalar field is analyzed for both negative and positive values of the cosmological term. In the first case, the Friedmann equation is studied both in…
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