The RS models and the subsequent generalization from a Minkowski brane to a Friedmann–Robertson–Walker
(FRW) brane [38, 260, 216, 226, 183, 330, 209, 145, 154] were derived as solutions in particular
coordinates of the 5D Einstein equations, together with the junction conditions at the Z_{2}-symmetric
brane^{2}.
A broader perspective, with useful insights into the inter-play between 4D and 5D effects, can be obtained
via the covariant Shiromizu–Maeda–Sasaki approach [388], in which the brane and bulk metrics remain
general. The basic idea is to use the Gauss–Codazzi equations to project the 5D curvature along the brane.
(The general formalism for relating the geometries of a spacetime and of hypersurfaces within that
spacetime is given in [423].)

The 5D field equations determine the 5D curvature tensor; in the bulk, they are

where represents any 5D energy-momentum of the gravitational sector (e.g., dilaton and moduli scalar fields, form fields).Let be a Gaussian normal coordinate orthogonal to the brane (which is at without loss of generality), so that , with being the unit normal. The 5D metric in terms of the induced metric on surfaces is locally given by

The extrinsic curvature of surfaces describes the embedding of these surfaces. It can be defined via the Lie derivative or via the covariant derivative: so that where square brackets denote anti-symmetrization. The Gauss equation gives the 4D curvature tensor in terms of the projection of the 5D curvature, with extrinsic curvature corrections: and the Codazzi equation determines the change of along via where .Some other useful projections of the 5D curvature are:

The 5D curvature tensor has Weyl (tracefree) and Ricci parts:

3.1 Field equations on the brane

3.2 5-dimensional equations and the initial-value problem

3.3 The brane viewpoint: A 1 + 3-covariant analysis

3.4 Conservation equations

3.5 Propagation and constraint equations on the brane

3.2 5-dimensional equations and the initial-value problem

3.3 The brane viewpoint: A 1 + 3-covariant analysis

3.4 Conservation equations

3.5 Propagation and constraint equations on the brane

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