In f(G,B) gravity the isotropy equation for stellar models is autonomous, and dynamical systems analysis of its phase portrait reveals stable invariant submanifolds.
Weinberg,Gravitation and Cosmology, Wiley, New York (1972)
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Dynamical systems approach to stellar modelling in $f(G, B)$ gravity
In f(G,B) gravity the isotropy equation for stellar models is autonomous, and dynamical systems analysis of its phase portrait reveals stable invariant submanifolds.