On the applicability of the level set method beyond the flamelet regime in thermonuclear supernova simulations
arXiv:astro-ph/0701416 · doi:10.1051/0004-6361:20066510
Abstract
In thermonuclear supernovae, intermediate mass elements are mostly produced by distributed burning provided that a deflagration to detonation transition does not set in. Apart from the two-dimensional study by Roepke & Hillebrandt (2005), very little attention has been payed so far to the correct treatment of this burning regime in numerical simulations. In this article, the physics of distributed burning is reviewed from the literature on terrestrial combustion and differences which arise from the very small Prandtl numbers encountered in degenerate matter are pointed out. Then it is shown that the level set method continues to be applicable beyond the flamelet regime as long as the width of the flame brush does not become smaller than the numerical cutoff length. Implementing this constraint with a simple parameterisation of the effect of turbulence onto the energy generation rate, the production of intermediate mass elements increases substantially compared to previous simulations, in which the burning process was stopped once the mass density dropped below 10^7 g/cm^3. Although these results depend on the chosen numerical resolution, an improvement of the constraints on the the total mass of burning products in the pure deflagration scenario can be achieved.
arXiv comment8 pages, 5 figures. Accepted for publication in Astron. & Astrophys
References in corpus (19)
- Type Ia Supernova Explosion: Gravitationally Confined Detonation
- Three-Dimensional Delayed-Detonation Model of Type Ia Supernova
- Constraints on the Physics of Type Ia Supernovae from the X-Ray Spectrum of the Tycho Supernova Remnant
- The Thermonuclear Explosion Of Chandrasekhar Mass White Dwarfs
- Deflagration to Detonation Transition in Thermonuclear Supernovae
- Late-Time Spectroscopy of SN 2002cx: The Prototype of a New Subclass of Type Ia Supernovae
- Constraints on the Progenitor Systems of Type Ia Supernovae
- A localised subgrid scale model for fluid dynamical simulations in astrophysics I: Theory and numerical tests
- Three-dimensional Numerical Simulations of Rayleigh-Taylor Unstable Flames in Type Ia Supernovae
- A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae
- Following multi-dimensional Type Ia supernova explosion models to homologous expansion
- Can Deflagration-Detonation-Transitions occur in Type Ia Supernovae?
- Multi-spot ignition in type Ia supernova models
- Direct Numerical Simulations of Type Ia Supernovae Flames II: The Rayleigh-Taylor Instability
- Low Carbon Abundance in Type Ia Supernovae
- The distributed burning regime in Type Ia supernova models
- Thermonuclear supernova simulations with stochastic ignition
- Level set simulations of turbulent thermonuclear deflagration in degenerate carbon and oxygen
- C+O detonations in thermonuclear supernovae: Interaction with previously burned material
Cited by in corpus (3)
- A three-dimensional deflagration model for Type Ia supernovae confronted with observations
- A Subgrid-scale Model for Deflagration-to-Detonation Transitions in Type Ia Supernova Explosion Simulations - Numerical implementation
- Turbulence in a 3D deflagration model for type Ia SNe: II. Intermittency and the deflagration-to-detonation transition probability