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Turbulence in a 3D deflagration model for type Ia SNe: II. Intermittency and the deflagration-to-detonation transition probability
W. Schmidt, F. Ciaraldi-Schoolmann, J. C. Niemeyer +2
The delayed detonation model describes the observational properties of the majority of type Ia supernovae very well. Using numerical data from a three-dimensional deflagration mode…
Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with M~0.9 M_sun
Ruediger Pakmor, Markus Kromer, Friedrich K. Roepke +3
Type Ia supernovae (SNe Ia) are thought to result from thermonuclear explosions of carbon-oxygen white dwarf stars. Existing models generally explain the observed properties, with…
The Diversity of Type Ia Supernovae from Broken Symmetries
Daniel Kasen, Fritz Roepke, S. E. Woosley
Type Ia supernovae result when carbon-oxygen white dwarfs in binary systems accrete mass from companion stars, reach a critical mass, and explode. The near uniformity of their ligh…
Turbulence in a three-dimensional deflagration model for Type Ia supernovae: I. Scaling properties
F. Ciaraldi-Schoolmann, W. Schmidt, J. C. Niemeyer +2
We analyze the statistical properties of the turbulent velocity field in the deflagration model for Type Ia supernovae. In particular, we consider the question of whether turbulenc…