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The data points show the signals predicted by our set of 2D and 3D Newtonian rotational core collapse models.
The goal of this project is to study axisymmetric, non-rotating stellar core collapse in full general relativity and to extract gravitational waves using light cone slicing.
Numerical simulations of supersonic jets are able to explain the structures observed in many VLA images of radio sources.
AMRA has been designed in such a way that virtually any numerical scheme can be easily used to solve the set of equations specific for certain problem.
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