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Supernova, nuclear synthesis, fluid instabilities, and interfacial mixing

Supernovae and their remnants are a central problem in astrophysics due to their role in the stellar evolution and nuclear synthesis. A supernova’s explosion is driven by a blast wave causing the development of Rayleigh–Taylor and Richtmyer–Meshkov instabilities and leading to intensive interfacial...

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Podrobná bibliografie
Vydáno v:Proc Natl Acad Sci U S A
Hlavní autoři: Abarzhi, Snezhana I., Bhowmick, Aklant K., Naveh, Annie, Pandian, Arun, Swisher, Nora C., Stellingwerf, Robert F., Arnett, W. David
Médium: Artigo
Jazyk:Inglês
Vydáno: National Academy of Sciences 2019
Témata:
On-line přístup:https://ncbi.nlm.nih.gov/pmc/articles/PMC6744890/
https://ncbi.nlm.nih.gov/pubmed/30478062
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1714502115
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