Comments on "Numerical Stability of Detonations in White Dwarf Simulations"
arXiv:1904.10001 · doi:10.1093/mnras/stz3285
Abstract
Katz & Zingale (2019, KZ19) recently studied a one-dimensional test problem, intended to mimic the process of detonation ignition in head-on collisions of two carbon--oxygen (CO) white dwarfs. They do not obtain ignition of a detonation in pure CO compositions unless the temperature is artificially increased or 5% He is included. In both of these cases they obtain converged ignition only for spatial resolutions better than 0.1 km, which are beyond the capability of multidimensional simulations. This is in a contradiction with the claims of Kushnir et al. (2013, K13), that a convergence to is achieved for a resolution of a few km. Using Eulerian and Lagrangian codes we show that a converged and resolved ignition is obtained for pure CO in this test problem without the need for He or increasing the temperature. The two codes agree to within 1% and convergence is obtained at resolutions of several km. We calculate the case that includes He and obtain a similar slow convergence, but find that it is due to a boundary numerical artifact that can (and should) be avoided. Correcting the boundary conditions allows convergence with resolution of in an agreement with the claims of K13. It is likely that the slow convergence obtained by KZ19 in this case is because of a similar boundary numerical artifact, but we are unable to verify this. KZ19 further recommended to avoid the use of the burning limiter introduced by K13. We show that their recommendation is not justified.
arXiv comment7 pages, 6 figures. Modified following referee report
References in corpus (13)
- Modules for Experiments in Stellar Astrophysics (MESA)
- Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
- Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
- Type Ia Supernova Explosion Models
- Observational clues to the progenitors of Type-Ia supernovae
- Extensible Component Based Architecture for FLASH, A Massively Parallel, Multiphysics Simulation Code
- Head-on collisions of white dwarfs in triple systems could explain type Ia supernova
- Equation of state of fully ionized electron-ion plasmas
- Failure of a neutrino-driven explosion after core-collapse may lead to a thermonuclear supernova
- Screening of fusion reactions from the principle of detailed balance and application to the reaction
- Numerical Stability of Detonations in White Dwarf Simulations
- Early Hydrodynamic Evolution of a Stellar Collision
- The structure of detonation waves in supernovae revisited
Cited by in corpus (4)
- Supernovae Ia in 2019 (review): a rising demand for spherical explosions
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- Quantifying Advantages of a Moving Mesh in Nuclear Hydrodynamics