2009

Holographic dark energy models: A comparison from the latest observational data

Li, Miao, Li, Xiao-Dong, Wang, Shuang et al.

Understand

The holographic principle of quantum gravity theory has been applied to the dark energy (DE) problem, and so far three holographic DE models have been proposed: the original holographic dark energy (HDE) model, the agegraphic dark energy (ADE) model, and the holographic Ricci dark energy (RDE) model.

In this work, we perform the best-fit analysis on these three models, by using the latest observational data including the Union+CFA3 sample of 397 Type Ia supernovae (SNIa), the shift parameter of the cosmic microwave background (CMB) given by the five-year Wilkinson Microwave Anisotropy Probe (WMAP5) observations, and the baryon acoustic oscillation (BAO) measurement from the Sloan Digital Sky Survey (SDSS).
The analysis shows that for HDE, $\chi_{min}^{2}=465.912$; for RDE, $\chi_{min}^{2}=483.130$; for ADE, $\chi_{min}^{2}=481.694$.
Among these models, HDE model can give the smallest $\chi^2_{min}$.

Built on

G. ’t Hooft, arXiv:gr-qc/9310026; L. Susskind, J. Math. Phys. 36
1995
Earlier work this paper cites.
J.R. Bond, G. Efstathiou and M. Tegmark, MNRAS. 291
1997
Earlier work this paper cites.
B. Ratra and P.J.E. Peebles, Phys. Rev. D 37
1999
Earlier work this paper cites.
A.G. Cohen, D.B. Kaplan and A.E. Nelson, Phys. Rev. Lett. 82
1999
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour and V. Mukhanov, Phys. Lett. B 458
2000
Earlier work this paper cites.
R.R. Caldwell, Phys. Lett. B 545
2003
Earlier work this paper cites.
T. Padmanabhan, Phys. Rev. D 66
2003
Earlier work this paper cites.
A.G. Riess et al., AJ. 116
2004
Earlier work this paper cites.
S.D.H. Hsu, Phys. Lett. B 594
2004
Earlier work this paper cites.
M. Li, Phys. Lett. B 603
2004
Earlier work this paper cites.
H. Wei, R.G. Cai, and D.F. Zeng, Class. Quant. Grav. 22
2005
Earlier work this paper cites.

Similar

D.J. Eisenstein et al., ApJ. 633
2005
Cited alongside, same era.
J. Simon, L. Verde, and R. Jimenez, Phys. Rev. D 71
2005
Cited alongside, same era.
M. Tegmark et al., Phys. Rev. D 69
2006
Cited alongside, same era.
S. Weinberg, Rev. Mod. Phys. 61
2006
Cited alongside, same era.
A.Y. Kamenshchik, U. Moschella and V. Pasquier, Phys. Lett. B 511
2006
Cited alongside, same era.
C.J. Feng, Phys. Lett. B 670
Original
2006
Cited alongside, same era.
Y. Wang and P. Mukherjee, ApJ. 650
2006
Cited alongside, same era.
C.L. Bennet et al., ApJS. 148, 1 (2003); D.N. Spergel et al., ApJS, 148, 175 (2003); D.N. Spergel et al., ApJS 170
2007
Cited alongside, same era.
R.G. Cai, Phys. Lett. B 657
2007
Cited alongside, same era.
Q.G. Huang and M. Li, JCAP 0408
2007
Cited alongside, same era.
E. Witten, arXiv:hep-ph/0002297
Cited in the paper.
C. Gao, F.Q. Wu, X.L. Chen and Y.G. Shen, arXiv:0712.1394
Original
Cited in the paper.

Then

S. Nesseris and L. Perivolaropoulos, Phys. Rev. D 72
2007
Later among the works it cites.
P. Mukherjee, D.R. Parkinson and A.R. Liddle, ApJ. 638
2007
Later among the works it cites.
Y. Zhang, T.Y. Xia, and W. Zhao, Class. Quant. Grav. 24
2008
Later among the works it cites.
H. Wei and R.G. Cai, Phys. Lett. B 660
2008
Later among the works it cites.
M. Kowalski et al., ApJ. 686
2008
Later among the works it cites.
Z.G. Dai, E.W. Liang and D. Xu, ApJL. 612
2008
Later among the works it cites.
S.W. Allen, et al, MNRAS. 353
2008
Later among the works it cites.
A.C.S. Friacas, J.S. Alcaniz, and J.A.S. Lima, MNRAS. 362
2008
Later among the works it cites.
H. Wei and R.G. Cai, Phys. Lett. B 655
Original
2009
Closest in time.
E. Komatsu et al., ApJS. 180
2009
Closest in time.

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