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Three-dimensional modeling has reached a level of maturity to providedetailed predictions of the gravitational wave emission in neutrino-driven corecollapse supernovae. We review the status of these modeling efforts, currentpredictions for core collapse supernova gravitational wave emission, and thestatus of algorithms for the detection of core collapse supernova gravitationalwaves and the estimation of physical parameters associated with these events,which we hope to use to cull information about the central engine.

Gravitational Waves from Neutrino-Driven Core Collapse Supernovae: Predictions, Detection, and Parameter Estimation