Spherically symmetric cosmology: resource paper

Abstract

We use the 1+3 frame formalism to write down the evolution equations for spherically symmetric models as a well-posed system of first order PDEs in two variables, suitable for numerical and qualitative analysis.

14 pages

References in corpus (1)

• Quasi-local variables in spherical symmetry: numerical applications to dark matter and dark energy sources

Cited by in corpus (4)

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• Averaging Generalized Scalar Field Cosmologies II: Locally Rotationally Symmetric Bianchi I and flat Friedmann-Lemaître-Robertson-Walker models