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arXiv · 2308.08299

GRDzhadzha: A code for evolving relativistic matter on analytic metric backgrounds

Josu C. Aurrekoetxea·Jamie Bamber·Sam E. Brady·Katy Clough·Thomas Helfer·James Marsden·Dina Traykova·Zipeng Wang
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Abstract

GRDzhadzha is an open-source code for relativistic simulations of matter fields on curved spacetimes that admit an analytic description (e.g. stationary black holes). It is based on the publicly available 3+1D numerical relativity code GRChombo. Such a description is valid where the density of the matter is small compared to the curvature scale of the spacetime, which is the case for many physical scenarios - for example, dark matter environments. The approach offers significant savings on memory and speed compared to running full numerical relativity simulations, since the metric variables and their derivatives are calculated analytically, and therefore are not evolved or stored on the grid. This brief paper introduces the code and gives details of some applications for which it has already been used.

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Josu C. Aurrekoetxea, Jamie Bamber, Sam E. Brady, Katy Clough, Thomas Helfer, James Marsden, Dina Traykova, Zipeng Wang. 2023-08-16. GRDzhadzha: A code for evolving relativistic matter on analytic metric backgrounds. https://arxiv.org/abs/2308.08299

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