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The proposal of pilgrim dark energy is based on the speculation thatphantom-like dark energy possesses enough resistive force to preclude the blackhole formation in the later universe. We explore this phenomenon by assumingthe generalized ghost version of pilgrim dark energy. We find that most of thevalues of the interacting ($\xi^2$) as well as pilgrim dark energy ($u$)parameters push the equation of state parameter towards phantom region. Thesquared speed of sound shows that this model remains stable in most of thecases of $\xi^2$ and $u$. We also develop $\omega_\Lambda-\omega'_\Lambda$plane and observe that this model corresponds to thawing as well as freezingregions. Finally, it is shown that the non-interacting and interactinggeneralized ghost versions of pilgrim dark energy correspond to $\Lambda$CDMlimit on the statefinder plane.

Analysis of Generalized Ghost Version of Pilgrim Dark Energy