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Phys. Rev. Lett. 92, 211102 (2004) [4 pages]

Deflagrations and Detonations in Thermonuclear Supernovae

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Vadim N. Gamezo1, Alexei M. Khokhlov2, and Elaine S. Oran1
1Laboratory for Computational Physics and Fluid Dynamics, Naval Research Laboratory, Washington, D.C. 20375, USA
2Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA

Received 16 January 2004; published 28 May 2004

We study a type Ia supernova explosion using three-dimensional numerical simulations based on reactive fluid dynamics. We consider a delayed-detonation model that assumes a deflagration-to-detonation transition. In contrast with the pure deflagration model, the delayed-detonation model releases enough energy to account for a healthy explosion, and does not leave carbon, oxygen, and intermediate-mass elements in central parts of a white dwarf. This removes the key disagreement between simulations and observations, and makes a delayed detonation the mostly likely mechanism for type Ia supernovae.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.92.211102
DOI:
10.1103/PhysRevLett.92.211102
PACS:
97.60.Bw, 26.30.+k, 47.40.–x, 47.70.Fw