Gravitational Wave Emission From Core-Collapse of Massive Stars

Abstract

We derive estimates for the characteristics of gravitational radiation from stellar collapse, using recent models of the core-collapse of Chandrasekhar mass white dwarfs (accretion induced collapse), core-collapse supernovae and collapsars, and the collapse of very massive stars (∼> 300M⊙). We study gravitational-wave emission mechanisms using several… (More)

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