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We present the analytical solutions for the evolution of matter density perturbations, for a model with a constant dark energy equation of state $w$ but when the effects of the dark energy perturbations are properly taken into account.
D. Sapone, E. Majerotto, M. Kunz and B. Garilli, Phys. Rev. D 88
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L. Amendola, M. Kunz and D. Sapone, JCAP 0804
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S. Nesseris and A. Mazumdar, Phys. Rev. D 79
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D. Sapone and M. Kunz, Phys. Rev. D 80
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A. B. Belloso, J. Garcia-Bellido and D. Sapone, JCAP 1110
2011
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J. Dossett and M. Ishak, Phys. Rev. D 88
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O. F. Piattella, D. L. A. Martins and L. Casarini, JCAP 1410
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2014
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2009
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D. Sapone, M. Kunz and L. Amendola, Phys. Rev. D 82
2010
Cited alongside, same era.
S. Nesseris, D. Sapone and J. Garcia-Bellido, arXiv:1410.0338 [astro-ph.CO]
Cited in the paper.
Cited in the paper.
A. Mehrabi, S. Basilakos and F. Pace, arXiv:1504.01262 [astro-ph.CO]
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Cited in the paper.
2015
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