Mathematical Simulation of Turbulent Combustion of Carbon in the Problems of White Dwarf Mergers and Explosions of Type Ia Supernovae
Author:
Publisher
Pleiades Publishing Ltd
Subject
Applied Mathematics,Industrial and Manufacturing Engineering
Link
https://link.springer.com/content/pdf/10.1134/S1990478921030066.pdf
Reference28 articles.
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3. S. Perlmutter, et al., “Measurements of the Cosmological Parameters $$\Omega $$ and $$\Lambda $$ from the First Seven Supernovae at $$z \geq 0.35 $$,” Astrophys. J. 483, 565–581 (1997).
4. S. Perlmutter, et al., “Measurements of $$\Omega $$ and $$\Lambda $$ from 42 High-Redshift Supernovae,” Astrophys. J. 517, 565–586 (1999).
5. W. Hillebrandt and J. Niemeyer, “Type Ia Supernova Explosion Models,” Ann. Rev. Astronomy and Astrophys. 38, 191–230 (2000).
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Mathematical Simulation of Nuclear Carbon Burning in White Dwarfs Using a 7-Isotope Reaction Network;Journal of Applied and Industrial Mathematics;2022-05
2. Mathematical Modeling of a High-Speed Collision of White Dwarfs—the Explosion Mechanism of Type Ia/Iax Supernovae;Journal of Applied and Industrial Mathematics;2022-02
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