On Some Recent Developments in Numerical Methods for Relativistic MHD

Physics

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Magnetohydrodynamics And Plasmas

Scientific paper

In recent years we have witnessed the rapid development of new numerical methods for Relativistic Magnetohydrodynamics. It is not going to be long before they become standard computational tools available to any keen researcher interested in relativistic astrophysics. In this paper I provide a very broad and yet brief review that is intended to help those who are not yet expert in the field, but who wish to become one in the future.

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