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Prog. Theor. Phys. Vol. 89 No. 6 (1993) pp. 1175-1182
Convective Instability in Hot Bubble in a Delayed Supernova Explosion
Shoichi Yamada,
Tetsuya Shimizu and
Katsuhiko Sato
Department of Physics, The University of Tokyo, Tokyo 113
(Received February 3, 1993)
Abstract:
Convective Instability behind a stalled shock wave is studied by performing a series of two-dimensional numerical simulations. This instability is induced by negative entropy gradient which is commonly formed in so-called “hot bubble” behind a stalled shock where matters are nearly hydrostatic and in radiative equilibrium. It is shown that an initial velocity perturbation of 1
URL :
http://ptp.ipap.jp/link?PTP/89/1175/
DOI : 10.1143/PTP.89.1175
References:
- M. Herant, W. Benz and S. Colgate, Ap. J. 395 (1992), 642.
- A. Burrows and B. A. Fryxell, Science 258 (1992), 430[Science].
- T.-H. Janka, to appear in the Proceedings of The International Symposium on Neutrino Astrophysics held in Takayama/Kamioka, Japan, on October 19-22, 1992.
- D. S. Miller, J. R. Wilson and R. W. Wilson, Ap. J. to be submitted.
- B. A. Fryxell, E. Müller and D. Arnett, Ap. J. 367 (1991), 619.
- I. Hachisu, T. Matsuda, K. Nomoto and T. Shigeyama, Ap. J. Lett. 358 (1990), L57.
- M. Den, T. Yoshida and Y. Yamada, Prog. Theor. Phys. 83 (1990), 723[PTP].
-
J. R. Wilson and R. W. Mayle, Phys. Rep. 163 (1988), 63[CrossRef].
- J. R. Wilson, R. W. Mayle, S. E. Woosley and T. Weaver, Ann. N. Y. Aca. Sci. 470 (1986), 267.
- S. Yamada and K. Sato, Ap. J. 382 (1991), 594.