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We explore a scenario of interacting dynamical dark energy model with the interaction term $Q$ including the varying equation-of-state parameter $w$.
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2013
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A. Lewis, “Efficient sampling of fast and slow cosmological parameters,” Phys. Rev. D 87
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G. Efstathiou, “ H 0 H_{0} revisited,” Mon. Not. Roy. Astron. Soc. 440
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D. N. Spergel, R. Flauger and R. Hložek, “Planck data reconsidered,” Phys. Rev. D 91
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