Schwarzschild geometry emerging from matrix models
Résumé
We demonstrate how various geometries can emerge from Yang-Mills type matrix models with branes, and consider the examples of Schwarzschild and Reissner-Nordström geometry. We provide an explicit embedding of these branes in R 2, 5 and R 4, 6, as well as an appropriate Poisson resp. symplectic structure which determines the non-commutativity of space-time. The embedding is asymptotically flat with asymptotically constant θ µν for large r, and therefore suitable for a generalization to many-body configurations. This is an illustration of our previous work [ 1 ], where we have shown how the Einstein-Hilbert action can be realized within such matrix models.
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