Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
Abdul Jawad, Shamaila Rani, Ines G. Salako, Faiza Gulshan

TL;DR
This paper explores new versions of pilgrim dark energy within the DGP braneworld model, analyzing cosmic acceleration and cosmological parameters, and finds results consistent with observational data supporting dark energy's role in accelerating the universe.
Contribution
It introduces and investigates new versions of pilgrim dark energy models in the DGP braneworld framework, analyzing their cosmological implications.
Findings
Equation of state indicates phantom-like behavior.
Deceleration parameter confirms accelerated expansion.
Cosmological diagnostics align with $ ext{Lambda CDM}$ model.
Abstract
The illustration of cosmic acceleration under two interacting dark energy models (pilgrim dark energy with Granda and Oliveros cutoff and its generalized ghost version) in DGP braneworld framework is presented. In the current scenario, the equation of state parameter, deceleration parameter, plane and statefinder diagnosis are investigated. The equation state parameter behave-like phantom era of the universe. The deceleration parameter depicts the accelerated expansion of the universe in both models. The cosmological planes like and statefinder corresponds to CDM limit. To end, we remark that our results support to phenomenon of pilgrim dark energy and cosmic acceleration. Also, the results are consistent with observational data.
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