Numerical solutions to Einstein's equation are constructed on compact non-orientable spatial slices for simple cosmological models with varying curvatures, including locally homogeneous and inhomogeneous examples, to test the methods and code.
Therefore the constants K and Λ must be chosen in a way that makes it possible for the integral of the right side of this equation to vanish as well
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Solving Einstein's Equation Numerically on Manifolds with Non-Orientable Spatial Slices
Numerical solutions to Einstein's equation are constructed on compact non-orientable spatial slices for simple cosmological models with varying curvatures, including locally homogeneous and inhomogeneous examples, to test the methods and code.