On the co-existence of matter dominated and accelerating solutions in f(G)-gravity and the case of f(R)-gravity

Mathematics – Functional Analysis

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Gravity, Cosmology, Dark Matter, Functional Analysis, Partial Differential Equations, Phenomenology Of Quantum Gravity, Origin And Formation Of The Universe, Dark Matter, Functional Analysis, Ordinary And Partial Differential Equations, Boundary Value Problems

Scientific paper

Working within the theory of modified Gauss-Bonnet gravity, we show that FLRW-like power-law solutions only exist for a very special class of f() theories. Furthermore, we point out that any transition from decelerated to accelerated expansion must pass through = 0, and no function f() that is differentiable at this point can admit both a decelerating power-law solution and any accelerating solution. This strongly constrains the cosmological viability of f()gravity, since it may not be possible to obtain an expansion history of the universe which is compatible with observations. We compare to the case of f(R)-gravity, and discuss possible caveats for the case of f()-gravity.

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