Table 1
Neutrino luminosities and average neutrino energy in hydrostatic simulations of the post bounce phase of a 30 solar mass progenitor.
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ED | 91.62 | 28.84 | 129.29 | 10.34 | 12.11 | 19.02 |
Foucart et al. (2016) | 82.55 | 23.00 | 82.48 | 8.72 | 10.90 | 22.83 |
Gray | 91.51 | 29.56 | 117.19 | 9.11 | 11.12 | 25.93 |
Notes. Each row represents a different neutrino transport scheme. The top row shows the results in the simulation with energy-dependent transport, and the following rows represent different iterations of the gray neutrino-transport scheme. Luminosities are denoted by L and average energies by 〈ε〉 with a subscript to denote the three different neutrino species.
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