Cosmological Evolution of Pilgrim Dark Energy in f(G) Gravity
Joint Authors
Source
Advances in High Energy Physics
Issue
Vol. 2015, Issue 2015 (31 Dec. 2015), pp.1-10, 10 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2015-03-10
Country of Publication
Egypt
No. of Pages
10
Main Subjects
Abstract EN
We analyze the behavior of pilgrim dark energy with Hubble horizon in f(G) gravity.
We reconstruct the f(G) models through correspondence phenomenon by assuming two values of pilgrim dark energy parameter (u=2, -2).
We evaluate the equation of state parameter which shows evolution of the universe in the quintessence, vacuum, and phantom phase for both cases of u and give favor the pilgrim dark energy phenomenon.
Also, squared speed of sound exhibits the stability of f(G) model for both cases of u.
The wPDE-wPDE′ also provides freezing and thawing regions in this scenario.
In this framework, the r-s plane also corresponds to different dark energy scenarios.
American Psychological Association (APA)
Jawad, Abdul& Rani, Shamaila. 2015. Cosmological Evolution of Pilgrim Dark Energy in f(G) Gravity. Advances in High Energy Physics،Vol. 2015, no. 2015, pp.1-10.
https://search.emarefa.net/detail/BIM-1052621
Modern Language Association (MLA)
Jawad, Abdul& Rani, Shamaila. Cosmological Evolution of Pilgrim Dark Energy in f(G) Gravity. Advances in High Energy Physics No. 2015 (2015), pp.1-10.
https://search.emarefa.net/detail/BIM-1052621
American Medical Association (AMA)
Jawad, Abdul& Rani, Shamaila. Cosmological Evolution of Pilgrim Dark Energy in f(G) Gravity. Advances in High Energy Physics. 2015. Vol. 2015, no. 2015, pp.1-10.
https://search.emarefa.net/detail/BIM-1052621
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-1052621