This work demonstrates spacetime symmetry impacts stability evaluation in cosmological models, emphasizing the fixed points and the Friedmann equation.
We define the iterative map from the metric gμν to the Einstein tensor Gμν as the Einstein Tensor Cycle (ETC) transformation, gμν(n+1):=Gμν[g(n)], and geometrically characterize Einstein spaces containing the cosmological constant Λ through its fixed points Gμν=λgμν. The FLRW metric’s fundamental symmetries—spatial isotropy (SO(3)) and spacetime homogeneity—are preserved under the ETC transformation and manifest as a fixed-point structure. We apply the ETC transformation to the FLRW metric with curvature parameters k=±1,0, analyzing how distinct spatial geometries are uniformly derived through a single iteration procedure. For the de Sitter family (H0=Λ/3), we confirm that G00=Λ and corresponding spatial components are realized in the first transformation and remain invariant in subsequent iterations for both k=+1 with a(t)=a0cosh(H0t) and k=−1 with a(t)=a0sinh(H0t). For the flat case (k=0), the Friedmann equation G00=8πGρ/c2 is reproduced under exponential expansion. The ETC transformation functions as a unified framework that simultaneously provides solution identification and stability evaluation in cosmological models, clarifying the deep relationship between spacetime symmetry and fixed-point structure.
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Hirokazu Maruyama (2025) studied this question.
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