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In this paper, we quantify the non-linear effects from $k$-essence dark energy through an effective parameter $\mu$ that encodes the additional contribution of a dark energy fluid or a modification of gravity to the Poisson equation.
1903
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1904
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1906
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C. Armendariz-Picon, V. F. Mukhanov and P. J. Steinhardt, A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration , Phys.Rev.Lett. 85
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A. Lewis, A. Challinor and A. Lasenby, Efficient computation of cosmic microwave background anisotropies in closed friedmann‐robertson‐walker models , The Astrophysical Journal 538
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C. Armendariz-Picon, V. F. Mukhanov and P. J. Steinhardt, Essentials of k essence , Phys. Rev. D63
2001
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2001
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M. Kunz and D. Sapone, Dark Energy versus Modified Gravity , Phys. Rev. Lett. 98
2007
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2011
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2012
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2016
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2012
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2015
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2015
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2016
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J. Lesgourgues, The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview , 1104.2932
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2017
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2018
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2018
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F. Hassani, J. Adamek, M. Kunz and F. Vernizzi, k-evolution: a relativistic n-body code for clustering dark energy , Journal of Cosmology and Astroparticle Physics 2019
2019
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