Abstract
The still unsolved puzzle of how to make a type II supernova explosion from the collapse of a massive star’s iron core, the detection of 19 neutrino events associated with SN 1987A in the 1MB and Kamiokande 2 experiments (BIONTA et al. [1], HIRATA et al. [2]) and, most currently, the idea of making nucleosynthesis by non- conservative scattering of neutrinos off heavy nuclei (EPSTEIN et al. [3]; WOOSLEY et al. [4]) keeps interest in neutrino emission from newly formed neutron stars very vivid.
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Janka, HT. (1991). Neutrino Transport in Supernovae and Protoneutron Stars by Monte Carlo Methods. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_57
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DOI: https://doi.org/10.1007/978-1-4612-2988-9_57
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