Interacting Ghost Dark Energy in Non-Flat Universe
A. Sheykhi, M. Sadegh Movahed

TL;DR
This paper explores a ghost dark energy model in a non-flat universe with interaction, analyzing its cosmological implications and fitting it to observational data to understand the universe's accelerated expansion.
Contribution
It extends the ghost dark energy model to include spatial curvature and interaction with dark matter, providing new insights into its equation of state and observational consistency.
Findings
Equation of state can be less than -1 with interaction
Model fits observational data with specific parameter values
Total energy density slightly exceeds flat universe value
Abstract
A new dark energy model called "ghost dark energy" was recently suggested to explain the observed accelerating expansion of the universe. This model originates from the Veneziano ghost of QCD. The dark energy density is proportional to Hubble parameter, , where is a constant of order and is QCD mass scale. In this paper, we extend the ghost dark energy model to the universe with spatial curvature in the presence of interaction between dark matter and dark energy. We study cosmological implications of this model in detail. In the absence of interaction the equation of state parameter of ghost dark energy is always and mimics a cosmological constant in the late time, while it is possible to have provided the interaction is taken into account. When , all previous results of ghost…
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