In our work we present results from numerical simulations of core collapse supernovae. We solve the general relativistic hydrodynamic equations, coupled to a dynamic (approximated) spacetime. Our computer code simulates the collapse of models of rotating stellar cores to nuclear matter densities. With a parameter study we identify and quantify the influence of relativistic effects, and compute the emitted gravitational wave signals. These so-called wave templates are an important tool for data analysis in gravitational wave detectors.
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In our work we present results from numerical simulations of core collapse supernovae. We solve the general relativistic hydrodynamic equations, coupled to a dynamic (approximated) spacetime. Our computer code simulates the collapse of models of rotating stellar cores to nuclear matter densities. With a parameter study we identify and quantify the influence of relativistic effects, and compute the emitted gravitational wave signals. These so-called wave templates are an important tool for data a...
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