Abstract
In this paper, we study the dynamics of self-gravitating fluid using structure scalars for spherical geometry in the context of f(G) cosmology. We construct structure scalars through orthogonal splitting of the Riemann tensor and deduce a complete set of equations governing the evolution of dissipative anisotropic fluid in terms of these scalars. We explore different causes of density inhomogeneity which turns out to be a necessary condition for viable models. It is explicitly shown that anisotropic inhomogeneous static spherically symmetric solutions can be expressed in terms of these scalar functions.
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Sharif, M., Fatima, H.I. Structure scalars and evolution equations in f(G) cosmology. Gen Relativ Gravit 49, 1 (2017). https://doi.org/10.1007/s10714-016-2163-x
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DOI: https://doi.org/10.1007/s10714-016-2163-x