The diversity of strongly interacting Type IIn supernovae

Open Access

Fig. 22.

Total neutrino energy contour plots. Top: contour plots of the total neutrino energy $ε_{ν + \bar{ν}}$ $\varepsilon_{\nu+\bar{\nu}}$ integrated for E_ν ≥ 1 TeV from Pitik et al. (2023) in function of the CSM radius and mass, over which the same parameters for our SNe are plotted. The orange star indicates the benchmark of the model. Bottom: same as above but in function of kinetic energy and CSM mass.

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