A Mechanism for a small but nonzero cosmological constant

TL;DR

This paper proposes a scalar field-based mechanism that explains a small, nonzero cosmological constant by modeling its decay over time and leveling off to mimic a true constant, aligning with recent cosmological observations.

Contribution

It introduces a novel model with two interacting scalar fields that produce a slowly leveling-off energy density, explaining the small, nonzero cosmological constant without fine-tuning.

Findings

The model achieves a decay of the effective cosmological constant as t^{-2}.

The total energy density levels off to mimic a constant Λ.

The parameters are linked to current and past cosmological data.

Abstract

Based on a thoeretical model in which scalar fields play crucial roles, we propose a mechanism to better understand a cosmological constant expected to be small (nearly comparable with the critical density) but nonzero as suggested strongly by the recent observations. We emphasize that a step further is needed beyond the simplest scenario of a decaying cosmological constant, according to which the effective $\Lambda$ is not a true constant but decays like $t^{-2}$, thus explaining why any effect of $\Lambda$ which is assumed to be of the Planckian order of magnitude in the earliest Universe is at most 120 orders smaller today ($t\sim 10^{60}$ in units of the Planck time), without any extreme fine-tuning of the parameters. In addition to the overall smooth fall-off $\sim t^{-2}$, the total energy density, the sum of the contributions from the ordinary matter and the scalar fields, must show some leveling-off behavior, hence mimicking a truly constant $\Lambda$ to fit the observations. We find that the desired behavior can be obtained by introducing two scalar fields interacting with each other in a specific manner. Many aspects of this model are discussed in detail, including the real origin of the whole mechanism, and how the parameters and the initial conditions of the theory can be determined by the cosomological parameters at the present epoch as well as the past history of the Universe.