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arXiv · 2409.03202

Generalized Ghost Dark Energy Model in Extended Modified Theory of Symmetric Telleparallel Gravity

M. Sharif·Iqra Ibrar
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Abstract

This paper focuses on developing a generalized ghost dark energy model $f\mathcal{(Q,T)}$ through the correspondence scheme for a non-interacting scenario involving pressureless matter and a power-law scale factor. We analyze the cosmological implications of our model using the equation of state parameter, $\omega_{GGDE}-\omega'_{GGDE}$ and the $r-s$ planes. We also examine stability of the model by considering squared speed of sound parameter. The equation of state parameter shows the phantom era, while the squared speed of sound indicates a stable generalized ghost dark energy model throughout the cosmic evolution. The $\omega_{GGDE}-\omega'_{GGDE}$ plane depicts a freezing region, whereas the $r-s$ plane corresponds to the Chaplygin gas model. We conclude that our results are consistent with the current observational data.

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M. Sharif, Iqra Ibrar. 2024-09-05. Generalized Ghost Dark Energy Model in Extended Modified Theory of Symmetric Telleparallel Gravity. https://arxiv.org/abs/2409.03202

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