Cosmological Evolution of Pilgrim Dark Energy in f(G)‎ Gravity

Joint Authors

Jawad, Abdul
Rani, Shamaila

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

Physics

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