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- W46961142 abstract "We present the gravitational wave signatures of three non-parameterized core collapse supernova explosion models for 12, 15, and 25 $M_{odot}$ non-rotating progenitors. The signatures exhibit four distinct stages. The third stage, induced by mass accretion onto the proto-neutron star owing to neutrino-driven convection and the SASI, dominates. The total gravitational wave energy emitted rises quickly as the SASI develops at ∼ 200 ms after bounce in all three models and levels off as explosion develops and the convection- and SASI-induced mass accretion powering the explosions and gravitational wave emission decreases. We decompose the gravitational wave signatures spectrally and show that the signal is within AdvLIGO’s bandpass for a Galactic event. The fundamental limitation of the current models and their associated predictions is the restriction to axisymmetry. Counterpart three-dimensional models are forthecoming." @default.
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- W46961142 date "2011-01-01" @default.
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- W46961142 title "Toward Computing the Gravitational Wave Signatures of Core Collapse Supernovae" @default.
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