One-Dimensional Numerical Study on Ignition of the Helium Envelope in Dynamical Accretion during the Double-Degenerate Merger
Kazuya Iwata, Keiichi Maeda

TL;DR
This study uses a one-dimensional hydrodynamic model to investigate helium envelope ignition in double-degenerate mergers, finding spontaneous detonation is unlikely for envelopes below 0.03 solar masses, but deflagration is more probable.
Contribution
It provides a self-consistent analysis of helium ignition thresholds in double-degenerate mergers, highlighting the limited conditions for spontaneous detonation and the potential for deflagration leading to DDT.
Findings
Spontaneous detonation requires helium envelope >~ 0.03 solar masses.
Deflagration is more likely for envelopes down to ~0.01 solar masses.
Composition mixing affects detonation likelihood and reaction rates.
Abstract
In order for a double-detonation model to be viable for normal type Ia supernovae, the adverse impact of helium-burning ash on early-time observables has to be avoided, which requires that the helium envelope mass should be at most 0.02 solar mass. Most of the previous studies introduced detonation by artificial hot spots, and therefore the robustness of the spontaneous helium detonation remains uncertain. In the present work, we conduct a self-consistent hydrodynamic study on the spontaneous ignition of the helium envelope in the context of the double-degenerate channel, by applying an idealized one-dimensional model and a simplified 7 isotope reaction network. We explore a wide range of the progenitor conditions, and demonstrate that the chance of direct initiation of detonation is limited. Especially, the spontaneous detonation requires the primary envelope mass of >~ 0.03 solar…
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Taxonomy
TopicsNuclear Physics and Applications · Combustion and Detonation Processes · Laser-Plasma Interactions and Diagnostics
