Abstract
The various mechanisms of dynamic instability onset at the last stages of stellar evolution are surveyed. The calculations of gravitational collapse of iron-oxygen stars are discussed. It is shown that there is no envelope ejection in this case, even when neutrino-nuclear coherent scattering is taken into account. The calculations of the carbon flash dynamics result in deflagrative regime of carbon burning. The carbon burning is finished up with formation of a collapsed, gravitationally bound, remnant when initial central density exceeds (3–5) 109 g cm−3. The modelling of the supernova outbursts gives us an evidence that the observational data for type I supernovae are well reproduced by slow (for several days) pumping of energy into envelope.
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Chechetkin, V.M., Imshennik, V.S., Ivanova, L.N., Nadyozhin, D.K. (1977). Gravitational Collapse, Weak Interactions, and Supernova Outbursts. In: Schramm, D.N. (eds) Supernovae. Astrophysics and Space Science Library, vol 66. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1229-4_15
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DOI: https://doi.org/10.1007/978-94-010-1229-4_15
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