Dong-Ze Xue | Searcharxiv

arXiv2017

Observational Constraints on Varying Alpha in $Λ(α)$CDM Cosmology

In this work, we consider the so-called $Λ(α)$CDM cosmology with $Λ\proptoα^{-6}$ while the fine-structure "constant" $α$ is varying. In this scenario, the accelerated expansion of the universe is driven by the cosmological "constant" $Λ$ (equivalently the vacuum energy), and the varying $α$ is driven by a subdominant scalar field $ϕ$ coupling with the electromagnetic field. The observational constraints on the varying $α$ and $Λ\proptoα^{-6}$ models with various couplings $B_F(ϕ)$ between the subdominant scalar field $ϕ$ and the electromagnetic field are considered.

gr-qc↗

arXiv2017

Cosmological Constant, Fine Structure Constant and Beyond

In the present work, we consider the cosmological constant model $Λ\proptoα^{-6}$, which is well motivated from three independent approaches. As is well known, the hint of varying fine structure constant $α$ was found in 1998. If $Λ\proptoα^{-6}$ is right, it means that the cosmological constant $Λ$ should also be varying. Here, we try to develop a suitable framework to model this varying cosmological constant $Λ\proptoα^{-6}$, in which we view it from an interacting vacuum energy perspective. Then, we consider the observational constraints on these models by using the 293 $Δα/α$ data from the absorption systems in the spectra of distant quasars. We find that the model parameters can be tightly constrained to the very narrow ranges of ${\cal O}(10^{-5})$ typically. On the other hand, we can also view the varying cosmological constant model $Λ\proptoα^{-6}$ from another perspective, namely it can be equivalent to a model containing "dark energy" and "warm dark matter", but there is no interaction between them. We find that this is also fully consistent with the observational constraints on warm dark matter.

gr-qc↗