
TL;DR
This paper investigates cosmological models within Weyl integrable spacetime, demonstrating that the scalar field can induce late-time accelerated expansion of the universe, acting as a phantom field under certain conditions.
Contribution
It introduces the role of the Weyl scalar field as a phantom field driving cosmic acceleration in homogeneous and isotropic cosmologies.
Findings
Weyl scalar field can act as a phantom field.
The model predicts late accelerated expansion for various initial conditions.
Acceleration occurs across a wide parameter range.
Abstract
We study homogeneous and isotropic cosmologies in a Weyl spacetime. It is shown that in Weyl integrable spacetime, the corresponding scalar field may act as a phantom field. In this circumstance the Weyl field gives rise to a late accelerated expansion of the Universe for all initial conditions and for a wide range of the parameters.
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