Abstract
Hydrodynamic instabilities play a key role in several astrophysical phenomena. We present a laser experiment related to the evolution of Rayleigh-Taylor instabilities (RTI) due to the passage of the shock wave through the He/H interface in a type II supernova. The experiment is performed on the CEA-Phébus laser facility and the RTI are studied using a bi-layer Cu/CH2 target with sinusoidal ripple at the interface.
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Arnett, D.: 1996, Supernovae and Nucleosyntesis, Princeton University Press, Princeton.
Baclet, Ph., Benuzzi-Mounaix, A., Bouquet, S., Cherfils, C., Chièze, J.-P., Muchielli, F., Munsch, P., Polès, L., Reverdin, Ch., Teyssier, R., Thais, F., Thébault, J.-P. and Troussel, Ph.: 1999, First International Conference on Inertial Fusion Science and Applications (IFSA'99), Sept. 12-17, Bordeaux, France.
Kumagai, S., Shigeyama, T., Nomoto, K., Itoh, M., Nishimura, J. and Tsuruta, S.: 1989, Astrophys. J. 345, 412-422.
Remington, B.A., Arnett, D., Drake, R.P. and Takabe, H.: 1999, Science 284, 1488-1493.
Remington, B.A., Kane, J., Drake, R.P., Glendinning, S.G., Estabrock, K., London, R., Castor, J., Wallace, R.J., Arnett, D., Liang, E., McCray, R., Rubenchick, A. and Fryxell, B.: 1997, Phys. Plasma 4, 1994-2003.
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Benuzzi-Mounaix, A., Bouquet, S., Chièze, JP. et al. Supernovae Rayleigh-Taylor Instability Experiments on the CEA-Phébus Laser Facility. Astrophysics and Space Science 277, 143–146 (2001). https://doi.org/10.1023/A:1012256801365
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DOI: https://doi.org/10.1023/A:1012256801365