A Three-Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations

doi:10.1086/521347

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F. K. Röpke et al. 2007 ApJ 668 1132 doi:10.1086/521347

A Three-Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations

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F. K. Röpke^1,2,3, W. Hillebrandt^1,3, W. Schmidt⁴, J. C. Niemeyer⁴, S. I. Blinnikov^1,5 and P. A. Mazzali^1,3,6

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Abstract References Cited By

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[9]: Turbulence in a Three-Dimensional Deflagration Model For Type Ia Supernovae. II. Intermittency and the Deflagration-to-Detonation Transition Probability
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[13]: Low Mach Number Modeling of Type IA Supernovae. IV. White Dwarf Convection
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[14]: Turbulence in a Three-Dimensional Deflagration Model for Type Ia Supernovae. I. Scaling Properties
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[15]: Spontaneous Initiation of Detonations in White Dwarf Environments: Determination of Critical Sizes
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[18]: Study of the Detonation Phase in the Gravitationally Confined Detonation Model of Type Ia Supernovae
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The Astrophysical Journal

The Astrophysical Journal

A Three-Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations

High-resolution Simulations of Convection Preceding Ignition in Type Ia Supernovae Using Adaptive Mesh Refinement

Nuclear astrophysics: the unfinished quest for the origin of the elements

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The Convective Phase Preceding Type Ia Supernovae

Type Ia Supernovae as Sites of the p-process: Two-dimensional Models Coupled to Nucleosynthesis

Formation of Dust in the Ejecta of Type Ia Supernovae

Simplified Hydrostatic Carbon Burning in White Dwarf Interiors

Nucleosynthesis in Two-Dimensional Delayed Detonation Models of Type Ia Supernova Explosions

Turbulence in a Three-Dimensional Deflagration Model For Type Ia Supernovae. II. Intermittency and the Deflagration-to-Detonation Transition Probability

Nebular Spectra and Explosion Asymmetry of Type Ia Supernovae

Shock Breakout from Type Ia Supernova

Adaptively Refined Large Eddy Simulations of a Galaxy Cluster: Turbulence Modeling and the Physics of the Intracluster Medium

Low Mach Number Modeling of Type IA Supernovae. IV. White Dwarf Convection

Turbulence in a Three-Dimensional Deflagration Model for Type Ia Supernovae. I. Scaling Properties

Spontaneous Initiation of Detonations in White Dwarf Environments: Determination of Critical Sizes

Pulsating Reverse Detonation Models of Type Ia Supernovae. II. Explosion

Pulsating Reverse Detonation Models of Type Ia Supernovae. I. Detonation Ignition

Study of the Detonation Phase in the Gravitationally Confined Detonation Model of Type Ia Supernovae

Astrophysical applications of the MAESTRO code

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Thermonuclear supernovae: a multi-scale astrophysical problem challenging numerical simulations and visualization

Flame-driven Deflagration-to-Detonation Transitions in Type Ia Supernovae?

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