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SASI Activity in Three-dimensional Neutrino-hydrodynamics Simulations of Supernova Cores

  • Authors: Florian Hanke, Bernhard Müller, Annop Wongwathanarat, Andreas Marek, and Hans-Thomas Janka

Hanke et al. 2013 The Astrophysical Journal 770 66.

  • Provider: AAS Journals

Caption: Figure 3.

Power spectra of v phiv of the 27  M 3D model sampled between r = 63 km and 80 km at post-bounce times of 222 ms (black) and 259 ms (red). At 222 ms, the strong SASI produces a distinctive peak at l = 1, which is absent during the later, convection-dominated phase.

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