Dynamics and Gravitational Wave Signature of Collapsar Formation
arXiv:1012.1853 · doi:10.1103/PhysRevLett.106.161103
Abstract
We perform 3+1 general relativistic simulations of rotating core collapse in the context of the collapsar model for long gamma-ray bursts. We employ a realistic progenitor, rotation based on results of stellar evolution calculations, and a simplified equation of state. Our simulations track self-consistently collapse, bounce, the postbounce phase, black hole formation, and the subsequent early hyperaccretion phase. We extract gravitational waves from the spacetime curvature and identify a unique gravitational wave signature associated with the early phase of collapsar formation.
4 pages, 4 figures, submitted to PRL
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