The core concept of general-relativistic model-building is that of a solution of Einstein’s equations. Given both Einstein’s equations and suitable equations for the properties of matter, such a solution consists of a specific semi-Riemannian manifold (usually defined by giving the metric in specific coordinates), and specific matter fields defined on that manifold.

Matter and geometry must satisfy Einstein’s equations, so in particular, the matter’s energy-momentum tensor must be divergence-free. The matter must, of course, also satisfy whatever additional equations were imposed on its properties. In short, such a solution is a model universe that satisfies the laws of general relativity, and possibly additional laws governing whatever matter might be present.

— Wikipedia on General relativity

2011.03.18 Friday ACHK

In mathematics and physics, n-dimensional anti de Sitter space, sometimes written AdSn, is a maximally symmetric Lorentzian manifold with constant negative scalar curvature. It is the Lorentzian analogue of n-dimensional hyperbolic space, just as Minkowski space and de Sitter space are the analogues of Euclidean and elliptical spaces respectively.

It is best known for its role in the AdS/CFT correspondence.

— Wikipedia on Anti de Sitter space

2011.03.16 Wednesday ACHK