428757.fig.0027a
(a)
428757.fig.0027b
(b)
428757.fig.0027c
(c)
Figure 27: spectra at the surface of the star in the case of (a), (b), and (c). We assume that the inverted mass hierarchy and . The solid lines (red lines) and the dotted lines (blue lines) are the spectra of polar direction and equatorial direction, respectively. Note in this figure that the neutrino luminosity and spectra are modeled to be the same as those obtained in a 1D full-scale numerical simulation by the Lawrence Livermore group [91]. These figures are taken from [305].