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2011

Thermodynamic of the Ghost Dark Energy Universe

Feng, Chao-Jun, Li, Xin-Zhou, Shen, Xian-Yong

Understand

Recently, the vacuum energy of the QCD ghost in a time-dependent background is proposed as a kind of dark energy candidate to explain the acceleration of the Universe.

In this model, the energy density of the dark energy is proportional to the Hubble parameter $H$, which is the Hawking temperature on the Hubble horizon of the Friedmann-Robertson-Walker (FRW) Universe.
In this paper, we generalized this model and choice the Hawking temperature on the so-called trapping horizon, which will coincides with the Hubble temperature in the context of flat FRW Universe dominated by the dark energy component.
We study the thermodynamics of Universe with this kind of dark energy and find that the entropy-area relation is modified, namely, there is an another new term besides the area term.

Built on

K. Kawarabayashi and N. Ohta, Nucl. Phys. B 175
1980
Earlier work this paper cites.
S. A. Hayward, Phys. Rev. D 49
1994
Earlier work this paper cites.
S. A. Hayward, Phys. Rev. D 53
1996
Earlier work this paper cites.
S. A. Hayward, Class. Quant. Grav. 15
1998
Earlier work this paper cites.
S. A. Hayward, S. Mukohyama and M. C. Ashworth, Phys. Lett. A 256
1999
Earlier work this paper cites.
R. G. Cai and S. P. Kim, JHEP 0502
2005
Earlier work this paper cites.
I. L. Shapiro, J. Sola and H. Stefancic, JCAP 0501
Original
2005
Earlier work this paper cites.
M. Akbar and R. G. Cai, Phys. Lett. B 635
2006
Earlier work this paper cites.
R. G. Cai and L. M. Cao, Phys. Rev. D 75
2007
Earlier work this paper cites.
M. Akbar and R. G. Cai, Phys. Lett. B 648
2007
Earlier work this paper cites.
A. Sheykhi,B. Wang and R. G. Cai, Nucl. Phys. B 779
2007
Earlier work this paper cites.