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Gravitational Waves from Core-Collapse Supernovae

Below we present GWs from our most recent simulations. We invite you to check out the repository at for GW generated by other groups.

Non-rotating progenitors

Series A

We present the gravitational wave signatures for a suite of core-collapse supernovae models. These models correspond to progenitors with masses in the range between 12 and 25 solar mass and are axisymmetric. More details of these simulations can be found in our paper Yakunin et al., 2010.