Supernovae and the Arrow of Time

Supernovae are explosions of stars and are a central problem in astrophysics. Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities develop during the star’s explosion and lead to intense interfacial RT/RM mixing of the star materials. We handle the mathematical challenges of the RT/RM probl...

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Detalles Bibliográficos
Autores principales: Abarzhi, Snezhana I., Hill, Desmon L., Naveh, Annie, Williams, Kurt C., Wright, Cameron E.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2022
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9223154/
https://www.ncbi.nlm.nih.gov/pubmed/35741549
http://dx.doi.org/10.3390/e24060829

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9223154/
https://www.ncbi.nlm.nih.gov/pubmed/35741549
http://dx.doi.org/10.3390/e24060829

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