Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications

Large-scale, three-dimensional numerical simulations of the deflagration stage of a thermonuclear supernova explosion show the formation and evolution of a highly convoluted turbulent flame in the gravitational field of an expanding carbon-oxygen white dwarf. The flame dynamics are dominated by the...

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Veröffentlicht in:	Science (American Association for the Advancement of Science) 2003-01, Vol.299 (5603), p.77-81
Hauptverfasser:	Gamezo, Vadim N., Khokhlov, Alexei M., Oran, Elaine S., Chtchelkanova, Almadena Y., Rosenberg, Robert O.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Climate Deflagration Earth, ocean, space Elementary particle and nuclear processes Energy Exact sciences and technology Flame propagation Flames Fundamental aspects of astrophysics Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Kinetics Late stages of stellar evolution (including black holes) Observations Physics Plumes Runaways Stars Stellar characteristics and properties Stellar structure, interiors, evolution, nucleosynthesis, ages Supernovae Supernovas Three dimensional modeling Turbulence Turbulent flames
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