Abstract
AbstractThe present study reports the bouncing cosmology of f(T) gravity with holographic Ricci form of density, that is, . Taking two forms of scale factor, namely exponential and power‐law, we have reconstructed f(T) gravity and accordingly derived expressions for the equation of state parameter in the bouncing scenario. The reconstructed equation of state parameter for the exponential form of scale factor showed a symmetric pattern about the turnaround point or bouncing point. Finally, we checked the stability of the models through the squared speed of sound and demonstrated how the stability depends upon the value of ξ.
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