Max-Planck Institute for Astrophysics

Three-dimensional simulations of an 27 solar-mass progenitor (2002 series of Alex Heger)

Model computed using the Lattimer&Swesty (K=220 MeV) equation of state and the neutrino transport employs 12 energy bins.

Model published in ApJ 770 (2013) 66 and arXiv:1303.6269

The following data is available

Movie: Time-evolution of the IceCube detection rate on a sky-plot of observer directions for the 27 M_sun supernova progenitor at 10 kpc.
The rate has been computed for the un-oscillated electron antineutrino flux (i.e., assuming no flavor conversions):

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