عنوان مجله
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Physics of the Dark Universe
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چکیده
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We study some cosmological features of Tsallis
holographic dark energy (THDE) in Cyclic, DGP and RS II braneworlds.
In our setup, a flat FRW universe is considered filled by a
pressureless source and THDE with the Hubble radius as the IR
cutoff, while there is no interaction between them. Our result shows
that although suitable behavior can be obtained for the system
parameters such as the deceleration parameter, the models are not
always stable during the cosmic evolution at the classical level.
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