A Low Matter Density Decaying Vacuum Cosmology from Complex Metric
Moncy V. John, K. Babu Joseph

TL;DR
This paper proposes a cosmological model where the universe's radius is a complex quantity, leading to a decaying vacuum scenario that addresses key cosmological problems and aligns with observational bounds.
Contribution
It introduces a novel complex metric approach to cosmology, deriving a scale factor that avoids singularities and solves classical cosmological issues.
Findings
The model predicts a finite initial radius comparable to the Planck length.
It confirms bounds on the current Hubble parameter consistent with observations.
The spacetime exhibits signature-changing properties and a peaked wave function in quantum cosmology.
Abstract
A low matter density decaying vacuum cosmology is proposed on the assumption that the universe's radius is a complex quantity \hat{R} if it is regarded as having a zero energy-momentum tensor. But we find that when the radius is real, it contains matter. Using the Einstein-Hilbert action principle, the physical scale factor R(t) =|\hat{R}| is obtained as equal to (R_0^{2} + t^{2})^{1/2} with R_0 representing the finite radius of the universe at t=0. The resulting physical picture is roughly a theoretical justification of the old Ozer-Taha model. The new model is devoid of all cosmological problems. In particular, it confirms the bounds on H_p, the present value of the Hubble parameter: 0.85 < H_p t_p < 1.91 and faces no age problem. We argue that the total energy density consists of parts corresponding to relativistic/non-relativistic matter, a positive vacuum energy and a form of…
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