Modified QCD Ghost Scalar Field Dark Energy in Anisotropic and Interacting Universe Models
DOI:
https://doi.org/10.26565/2312-4334-2025-4-04Keywords:
Bianchi type-III, QCD ghost dark energy, Cold dark matter, Scalar field modelsAbstract
In this work, we study the Bianchi type-III interacting framework of modified QCD ghost dark energy with cold dark matter is being considered for illustrating the accelerated expansion of the Universe. The equation of state parameter shows evolution of the universe completely varies in quintessence region only. The dynamics of scalar field and corresponding potential of various scalar field models shows consistence behavior with the accelerated expansion phenomenon. Also, the kinetic energy term of k-essence models lies within the range where equation of state parameter represents the accelerated expansion of the Universe.
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