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2012

Fingerprinting Dark Energy III: distinctive marks of viscosity

Sapone, Domenico, Majerotto, Elisabetta

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The characterisation of dark energy is one of the primary goals in cosmology especially now that many new experiments are being planned with the aim of reaching a high sensitivity on cosmological parameters.

It is known that if we move away from the simple cosmological constant model then we need to consider perturbations in the dark energy fluid.
This means that dark energy has two extra degrees of freedom: the sound speed $\cs$ and the anisotropic stress $\sigma$.
If dark energy is inhomogenous at the scales of interest then the gravitational potentials are modified and the evolution of the dark matter perturbations is also directly affected.

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Built on

D. N. Limber, Astrophys. J. 119
1954
Earlier work this paper cites.
R. K. Sachs and A. M. Wolfe, Astrophys. J. 147
1967
Earlier work this paper cites.
H. Kodama and M. Sasaki, Prog. Theor. Phys. Suppl. 78
1984
Earlier work this paper cites.
R. Durrer, Fund. Cosmic Phys. 15
1994
Earlier work this paper cites.
C. P. Ma and E. Bertschinger, Astrophys. J. 455
1995
Earlier work this paper cites.
W. Hu, D. N. Spergel and M. J. White, Phys. Rev. D 55
1997
Earlier work this paper cites.
A. G. Riess et al., Astronomical J. 116
1998
Earlier work this paper cites.
W. Hu, Astrophys. J. 506
1998
Earlier work this paper cites.
S. Perlmutter et al., Astrophys. J. 517
1999
Earlier work this paper cites.
D. Eisenstein & W. Hu, Astrophys. J. 511
1999
Earlier work this paper cites.

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Then

B. M. Schäfer, arXiv:0803.2239 (2008)
Original
2008
Later among the works it cites.
D. Sapone, M. Kunz Phys. Rev. D 80
Original
2009
Later among the works it cites.
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Original
2009
Later among the works it cites.
J. B. Dent, S. Dutta, T. J. Weiler, Phys. Rev. D 79
2009
Later among the works it cites.
J. B. Dent, S. Dutta, L. Perivolaropoulos, Phys. Rev. D 80
2009
Later among the works it cites.
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