Direct numerical simulations of type Ia supernovae flames II: The Rayleigh-Taylor instability
- LBNL Library
A Type Ia supernova explosion likely begins as a nuclear runaway near the center of a carbon-oxygen white dwarf. The outward propagating flame is unstable to the Landau-Darrieus, Rayleigh-Taylor, and Kelvin-Helmholtz instabilities, which serve to accelerate it to a large fraction of the speed of sound. We investigate the Rayleigh-Taylor unstable flame at the transition from the flamelet regime to the distributed-burning regime, around densities of 10e7 gm/cc, through detailed, fully resolved simulations. A low Mach number, adaptive mesh hydrodynamics code is used to achieve the necessary resolution and long time scales. As the density is varied, we see a fundamental change in the character of the burning--at the low end of the density range the Rayleigh-Taylor instability dominates the burning, whereas at the high end the burning suppresses the instability. In all cases, significant acceleration of the flame is observed, limited only by the size of the domain we are able to study. We discuss the implications of these results on the potential for a deflagration to detonation transition.
- Research Organization:
- Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, CA (US)
- Sponsoring Organization:
- USDOE Director. Office of Science. Office of Computational and Technology Research. Mathematics Information and Computational Sciences Division, Supernova Science Center/UCSC Contract DE-FC02-01ER41176 and DE-AC05-00OR22725; National Aeronautics and Space Administration Award NAG5-12036, National Science Foundation MRI Grant AST-0079757 (US)
- DOE Contract Number:
- AC03-76SF00098
- OSTI ID:
- 841916
- Report Number(s):
- LBNL--54300
- Journal Information:
- Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: pt.1 Vol. 608
- Country of Publication:
- United States
- Language:
- English
Similar Records
Three-dimensional numerical simulations of Rayleigh-Taylorunstable flames in type Ia supernovae
GRAVITATIONALLY UNSTABLE FLAMES: RAYLEIGH-TAYLOR STRETCHING VERSUS TURBULENT WRINKLING
Rayleigh-Taylor and Kelvin-Helmholtz instabilities in targets accelerated by laser ablation
Journal Article
·
Thu Jan 27 23:00:00 EST 2005
· Astrophysical Journal
·
OSTI ID:862068
GRAVITATIONALLY UNSTABLE FLAMES: RAYLEIGH-TAYLOR STRETCHING VERSUS TURBULENT WRINKLING
Journal Article
·
Wed Jul 10 00:00:00 EDT 2013
· Astrophysical Journal
·
OSTI ID:22140130
Rayleigh-Taylor and Kelvin-Helmholtz instabilities in targets accelerated by laser ablation
Journal Article
·
Sun Mar 07 23:00:00 EST 1982
· Phys. Rev. Lett.; (United States)
·
OSTI ID:5381103
Related Subjects
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ACCELERATION
EXPLOSIONS
FLAMES
HYDRODYNAMICS
INSTABILITY
MACH NUMBER
RAYLEIGH-TAYLOR INSTABILITY
RESOLUTION
SUPERNOVAE
SUPERNOVAE: GENERAL WHITE DWARFS HYDRODYNAMICS NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES CONDUCTION METHODS: NU MERICAL
VELOCITY
GENERAL PHYSICS
ACCELERATION
EXPLOSIONS
FLAMES
HYDRODYNAMICS
INSTABILITY
MACH NUMBER
RAYLEIGH-TAYLOR INSTABILITY
RESOLUTION
SUPERNOVAE
SUPERNOVAE: GENERAL WHITE DWARFS HYDRODYNAMICS NUCLEAR REACTIONS NUCLEOSYNTHESIS ABUNDANCES CONDUCTION METHODS: NU MERICAL
VELOCITY