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3 Collapse of Massive Stars


 3.1 Collapse scenario
 3.2 Formation rate
 3.3 GW emission mechanisms
 3.4 Numerical predictions of GW emission
  3.4.1 Historical investigations
  3.4.2 Axisymmetric simulations
  3.4.3 Non-axisymmetric simulations
  3.4.4 General relativistic simulations
  3.4.5 Simulations of convective instabilities
 3.5 Going further

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