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We consider the cosmology of the Ricci-tensor-squared gravity in the Palatini variational approach.
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Here Q a k = a k ∇ ^ a Q k Q^{k}_{a}=\frac{a}{k}\hat{\nabla}_{a}Q^{k} and Q k Q^{k} is the zero order eigenfunction of the comoving Laplacian a 2 ∇ ^ 2 a^{2}\hat{\nabla}^{2} ( a 2 ∇ ^ 2 Q k = k 2 Q k a^{2}\hat{\nabla}^{2}Q^{k}=k^{2}Q^{k} ), with eigenvalue k 2 k^{2} , k k representing a specified scale
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