Quick Search:
Author: Title/Abstract: Vol./No: Page:

Prog. Theor. Phys. Vol. 86 No. 6 (1991) pp. 1211-1225

[ Full Text PDF : FREE ACCESS (746K) ]

Two-Dimensional Simulations of Hydrodynamic Instability in Supernova Explosion. II

Yoshiyuki Yamada, Tatsuo Yoshida* and Mitsue Den

Department of Physics, Kyoto University, Kyoto 606
*Department of Physics, Hokkaido University, Sapporo 060

(Received June 10, 1991)

Abstract:

Mechanism of global mixing in supernova ejecta is analyzed numerically. An axisymmetric system of hydrodynamic equations is solved using Eulerian scheme for various types of initial perturbations. We confirm the non-linear growth of perturbations near the H/He interface. We find that the reverse shock generated from the interaction between the blast shock and the H/He interface is essential for the growth of perturbations near the He/C + O interface. The perturbation near the He/C + O interface decays due to the interaction with the reverse shock. We conclude that a substantial amount of perturbations is required if the initial seed is originated from inside the He burning shell.


URL : http://ptp.ipap.jp/link?PTP/86/1211/
DOI : 10.1143/PTP.86.1211

[ Full Text PDF : FREE ACCESS (746K) ] Citation:


References:

  1. T. Dotani et al., Nature 30 (1987), 230.
    R. Sunyaev et al., Nature 330 (1987), 227[CrossRef].
  2. T. Shigeyama and K. Nomoto, in the Proceedings of the Tenth Santa Cruz Summer Workshop on Supernova”, ed. S. E. Woosley (Springer Verlag, N.Y., 1990), p. 198.
  3. F. C. Witteborn et al., Astrophys. J. Lett. 338 (1989), L9[CrossRef].
  4. M. Den, T. Yoshida and Y. Yamada, Prog. Theor. Phys. 83 (1990), 723[PTP].
  5. M. Nagasawa, T. Nakamura and S. M. Miyama, Publ. Astron. Soc. Jpn. 40 (1988), 691.
  6. E. Müller, W. Hillebrandt, M. Orio, P. Höflich, R. Mönchmeyer and B. A. Fryxell, Astron. Astrophys. 220 (1989), 167.
  7. M. Nagasawa, preprint.
  8. W. Bentz and F.-K. Thielemann, Bull. A. A. S. 20 (1989), 985.
  9. Y. Yamada, T. Nakamura and K. Oohara, Prog. Theor. Phys. 84 (1990), 436[PTP].
  10. D. Arnett, B. Fryxell and E. Müller, Astrophys. J. Lett. 341 (1989), L63[CrossRef].
  11. B. Fryxell, E. Müller and D. Arnett, Astrophys. J. 367 (1991), 619[CrossRef].
  12. I. Hachisu, T. Matsuda, K. Nomoto and T. Shigeyama, Astrophys. J. Lett. 358 (1990), L58.
  13. I. Hachisu, T. Matsuda, K. Nomoto and T. Shigeyama, Astrophys. J. Lett. 368 (1991), L27[CrossRef].
  14. R. A. Chevalier, Astrophys. J. 207 (1976), 872[CrossRef].