Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.3902f&link_type=abstract
American Astronomical Society, 196th AAS Meeting, #39.02; Bulletin of the American Astronomical Society, Vol. 32, p.735
Astronomy and Astrophysics
Astrophysics
Scientific paper
We compare two and three-dimensional simulations of the cellular structure of carbon detonations. The initial density of the carbon is taken to be 107 g cm-3. This value has been suggested as the density at which a deflagration to detonation transition may occur in Type Ia supernovae. An initial planar detonation front becomes unstable and develops a complex structure due to the generation of transverse waves. Differences in the amount of asymmetry between the 2D and 3D cases, as well as the relative sizes of individual cells will be discussed. This work was supported in part by the Department of Energy Grant No. B341495 to the Center for Astrophysical Thermonuclear Flashes at the University of Chicago under the ASCI Strategic Alliances Program.
Calder Alan C.
Dursi Jonathan L.
Fryxell Bruce
MacNeice Peter
Olson Kevin
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