Abstract
We analyze pilgrim dark energy model in the background of f(R) gravity by taking IR cut-offs as particle and event horizons as well as conformal age of the universe. We regard the f(R) theory as an effective description for the pilgrim dark energy and reconstruct the function f(R) with the parameter μ<0 (which supports the phantom regime). Finally, we show the distinctive behavior of f(R) for the future cosmic evolution.
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