Rip cosmological models in extended symmetric teleparallel gravity

Abstract

In this paper we have investigated some rip cosmological models in an extended symmetric teleparallel gravity theory. We consider the form $f(Q,T)=a{Q}^m+bT$ in the Einstein-Hilbert action and expressed the field equations and the dynamical parameters in terms of the non-metricity $Q$. Three rip models such as Little Rip, Big Rip and Pseudo Rip are presented. The energy conditions and the cosmographic parameters are derived and analysed for all these models.

arXiv comment14 pages, 18 figures, Accepted for publication in Physics of the Dark Universe

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• Scalar field source Teleparallel Robertson-Walker F(T)-gravity solutions
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