Abstract

We study effects of cosmic fluids on finite-time future singularities in modified f(R,G)f(R,G)-gravity, where RR and GG are the Ricci scalar and the Gauss-Bonnet invariant, respectively. We consider the fluid equation of state in the general form, ω=ω(ρ)\omega=\omega(\rho), and we suppose the existence of a bulk viscosity. We investigate quintessence region (ω>1\omega>-1) and phantom region (ω<1\omega<-1) and the possibility to change or avoid the singularities in f(R,G)f(R,G)-gravity. Finally, we study the inclusion of quantum effects in large curvatures regime.Comment: 14 page

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    Last time updated on 05/06/2019