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The CHIMERA code is a multi-dimensional multi-physics engine dedicatedprimarily to the simulation of core collapse supernova explosions. One of themost important aspects of these explosions is their capacity to producegravitational radiation that is detectable by Earth-based laser-interferometricgravitational wave observatories such as LIGO and VIRGO. We present herepreliminary gravitational signatures of two-dimensional models withnon-rotating progenitors. These simulations exhibit explosions, which arefollowed for more than half a second after stellar core bounce.

Core Collapse Supernovae using CHIMERA: Gravitational Radiation from Non-Rotating Progenitors