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
http://www.livingreviews.org/lrr-2003-2
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