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In the delayed explosion scenario of core-collapse supernovae (SNe), the accretion phase shows pronounced convective overturns and a low-multipole hydrodynamic instability, the standing accretion shock instability (SASI).
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A. Burrows, L. Dessart, C. D. Ott and E. Livne, “Multi-dimensional explorations in supernova theory,” Phys. Rept. 442
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A. Burrows, L. Dessart, E. Livne, C. D. Ott and J. Murphy, “Simulations of magnetically driven supernova and hypernova explosions in the context of rapid rotation,” Astrophys. J. 664
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A. Burrows, E. Livne, L. Dessart, C. D. Ott and J. Murphy, “Features of the acoustic mechanism of core-collapse supernova explosions,” Astrophys. J. 655
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2009
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C. D. Ott, “The gravitational wave signature of core-collapse supernovae,” Class. Quant. Grav. 26
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2010
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2010
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