Abstract
Although over the last fifteen years many authors have investigated the question of whether or not the gravitational collapse of the cores of highly evolved massive stars (M ≳ 10 MƟ) can give rise to the observed (type II) supernova events, the problem has not been solved yet, despite the fact that the general ideas are quite simple and convincing.
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Hillebrandt, W. (1982). Computer Simulations of Stellar Collapse and Supernovae Explosions: Non-Rotating and Rotating Models. In: Rees, M.J., Stoneham, R.J. (eds) Supernovae: A Survey of Current Research. NATO Advanced Study Institutes Series, vol 90. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7876-8_7
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