For power-law f(G) gravity, the matter power spectrum computed from 1+3 covariant perturbations is not scale invariant, with curves decaying and then rising above the GR flat line as k grows.
A Covariant Approach to 1+3 Formalism
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abstract
I present a covariant approach to developing 1+3 formalism without an introduction of any basis or coordinates. In the formalism, a spacetime which has a timelike congruence is assumed. Then, tensors are split into temporal and spatial parts according to the tangent direction to the congruence. I make use of the natural derivatives to define the kinematical quantities and to investigate their properties. They are utilized in the splitting of covariant derivatives. In this way, the Riemann curvature is split into the temporal and spatial part, i.e. Gauss, Codazzi, and Ricci relation. Finally, the splitting of the Einstein equation is achieved by contraction. Choosing congruence as normal to a spacelike hypersurface, the formalism reduces to 3+1 formalism. This approach deepens our understanding of 3+1 formalism. All these processes are performed in a covariant manner without the complexities caused by the introduction of a coordinate system or basis.
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Matter power spectrum in a power-law $f(G)$ gravity
For power-law f(G) gravity, the matter power spectrum computed from 1+3 covariant perturbations is not scale invariant, with curves decaying and then rising above the GR flat line as k grows.