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Paper detail

Radiation from a D-dimensional collision of shock waves: numerical methods

We present a pedagogical introduction to the problem of evolving a head on collision of two Aichelburg-Sexl gravitational shock waves in D-dimensions, using perturbative techniques. We follow a constructive approach with examples, going in some detail through: the set up of the exact initial conditions and their properties; perturbative methods in flat space-time with Green function solutions; and numerical strategies to evaluate the integral solutions. We also discuss, briefly, radiation extraction methods adapted to this problem, together with some of the results for this system.

preprint2013arXivOpen access
Marco O. P. Sampaio
hep-phgr-qchep-th
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Marco O. P. Sampaio

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