Presents an observer-explicit diagnostic framework that separates inhomogeneity, expansion variance, shear, and Weyl curvature contributions in cosmological solutions of Einstein's equations, tested on six benchmark families with public code.
Modelling inhomogeneity in Szekeres spacetime,
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Geometric Phase-Space Structure in Cosmological Solutions of Einstein's Field Equations
Presents an observer-explicit diagnostic framework that separates inhomogeneity, expansion variance, shear, and Weyl curvature contributions in cosmological solutions of Einstein's equations, tested on six benchmark families with public code.