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Advances in High Energy Physics
Volume 2015, Article ID 952156, 10 pages
Research Article

Cosmological Evolution of Pilgrim Dark Energy in Gravity

Department of Mathematics, COMSATS Institute of Information Technology, Lahore 54000, Pakistan

Received 4 January 2015; Revised 21 February 2015; Accepted 1 March 2015

Academic Editor: Elias C. Vagenas

Copyright © 2015 Abdul Jawad and Shamaila Rani. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


We analyze the behavior of pilgrim dark energy with Hubble horizon in gravity. We reconstruct the models through correspondence phenomenon by assuming two values of pilgrim dark energy parameter . We evaluate the equation of state parameter which shows evolution of the universe in the quintessence, vacuum, and phantom phase for both cases of and give favor the pilgrim dark energy phenomenon. Also, squared speed of sound exhibits the stability of model for both cases of . The also provides freezing and thawing regions in this scenario. In this framework, the plane also corresponds to different dark energy scenarios.