Fetching the paper…
Reading the bibliography…
In this paper, we compare some popular dark energy models under the assumption of a flat universe by using the latest observational data including the type Ia supernovae Constitution compilation, the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey, the cosmic microwave background measurement given by the seven-year Wilkinson Microwave Anisotropy Probe observations and the determination of $H_0$ from the Hubble Space Telescope.
A. Einstein, Cosmological Considerations in the General Theory of Relativity,
1917
Earlier work this paper cites.
1932
Earlier work this paper cites.
H. Akaike, A new look at the statistical model identification,
1974
Earlier work this paper cites.
G. Schwarz, Estimating the Dimension of a Model,
1978
Earlier work this paper cites.
P. J. E. Peebles and B. Ratra, Cosmology With A Time Variable Cosmological ’Constant’,
1995
Earlier work this paper cites.
W. Hu and N. Sugiyama, Small scale cosmological perturbations: An Analytic approach,
1996
Earlier work this paper cites.
J. R. Bond, G. Efstathiou and M. Tegmark, Forecasting Cosmic Parameter Errors from Microwave Background Anisotropy Experiments,
1997
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
A. G. Cohen, D. B. Kaplan and A. E. Nelson, Effective field theory, black holes, and the cosmological constant,
1999
Earlier work this paper cites.
G. R. Dvali, G. Gabadadze and M. Porrati, 4D gravity on a brane in 5D Minkowski space,
2000
Earlier work this paper cites.
A. Y. Kamenshchik, U. Moschella and V. Pasquier, An alternative to quintessence,
2002
Earlier work this paper cites.
M. C. Bento, O. Bertolami and A. A. Sen, Generalized Chaplygin gas, accelerated expansion and dark energy-matter unification,
2002
Earlier work this paper cites.
S. Weinberg, The cosmological constant problem,
2003
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter,
2003
Earlier work this paper cites.
M. Li, A model of holographic dark energy,
2004
Earlier work this paper cites.
Q. G. Huang and M. Li, The holographic dark energy in a non-flat universe,
2004
Earlier work this paper cites.
A. R. Liddle, How many cosmological parameters?,
2004
Cited alongside, same era.
T. D. Saini, J. Weller and S. L. Bridle, Revealing the Nature of Dark Energy Using Bayesian Evidence,
2004
Cited alongside, same era.
X. Zhang, F. Q. Wu and J. Zhang, New Generalized Chaplygin Gas as a Scheme for Unification of Dark Energy and Dark Matter,
2005
Cited alongside, same era.
D. J. Eisenstein et al
2005
Cited alongside, same era.
W. Godlowski and M. Szydlowski, Which cosmological model with dark energy – phantom or LambdaCDM,
2006
Cited alongside, same era.
R. G. Cai, A Dark Energy Model Characterized by the Age of the Universe,
2007
B. Jain and P. Zhang, Observational Tests of Modified Gravity,
2008
Later among the works it cites.
H. Wei and R. G. Cai, Cosmological Constraints on New Agegraphic Dark Energy,
2008
Later among the works it cites.
2009
Closest in time.
R. G. Cai, B. Hu and Y. Zhang, Holography, UV/IR Relation, Causal Entropy Bound and Dark Energy,
2009
Closest in time.
2009
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
Cited alongside, same era.
2007
Cited alongside, same era.
T. M. Davis et al
2007
Cited alongside, same era.
A. R. Liddle, Information criteria for astrophysical model selection,
2007
Cited alongside, same era.
S. Nesseris and L. Perivolaropoulos, Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models,
2007
Cited alongside, same era.
Y. Wang and P. Mukherjee, Observational Constraints on Dark Energy and Cosmic Curvature,
2007
Cited alongside, same era.
H. Wei and R. G. Cai, A New Model of Agegraphic Dark Energy,
2008
Cited alongside, same era.
Closest in time.
2009
Closest in time.
2009
Closest in time.
2009
Closest in time.
2009
Closest in time.
X. Zhang and F. Q. Wu, Constraints on holographic dark energy from type Ia supernova observations,
2009
Closest in time.
2009
Closest in time.
2009
Closest in time.
2010
Closest in time.
2010
Closest in time.