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Supernova Explosions - The Role of a Rayleigh-Taylor Instability
Published online by Cambridge University Press: 12 April 2016
Abstract
A two dimensional hydrodynamic study indicates that convectively unstable gradients which develop during core collapse and bounce give rise to large scale core overturn. It is also shown that the concomitant release of neutrini can deposit large amounts of energy and momentum in the infalling envelope and give rise to a powerful supernova explosion.
- Type
- IX. Supernovae
- Information
- International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 571 - 577
- Copyright
- Copyright © Reidel 1980