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6.3 GW emission mechanisms

The GW emission mechanisms related to the collapse of SMSs are a subset of those discussed in the sections on AIC, SNe/collapsars, and Population III stellar collapse. These include (i) aspherical collapse, (ii) global rotational and fragmentation instabilities that may arise during the collapse/explosion and in the collapsed remnant (prior to black hole formation), and (iii) the “ring-down” of the remnant black hole.
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