Chaos and turbulent nucleosynthesis prior to a supernova explosion
Three-dimensional (3D), time dependent numerical simulations of flow of matter in stars, now have sufficient resolution to be fully turbulent. The late stages of the evolution of massive stars, leading up to core collapse to a neutron star (or black hole), and often to supernova explosion and nucleo...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
AIP Publishing LLC
2014-03-01
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| Series: | AIP Advances |
| Online Access: | http://dx.doi.org/10.1063/1.4867384 |