Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation

TL;DR

This study uses high-resolution 3D simulations to determine the impact-parameter threshold for detonations in white dwarf collisions, considering various initial conditions and their effects on supernova outcomes.

Contribution

It introduces a detonation criterion based on impact parameter for both direct and indirect white dwarf collisions using advanced 3D simulations.

Findings

Detonation threshold depends on impact parameter, density, composition, and velocity.

Initial velocity significantly influences 56Ni production.

Numerical modeling aspects affect the amount of 56Ni synthesized.

Abstract

The physical collisions of two white dwarfs (WDs) (i.e. not slow mergers) have been shown to produce type-Ia-like supernovae (SNe) explosions. Most studies of WD collisions have focused on zero impact-parameter (direct) collisions, which can also be studied in 2D. However, the vast majority of WD collisions arising from any evolutionary channels suggested to date are expected to be indirect, i.e. have a non-negligible impact parameter upon collision. Here, we use one of the highest resolution 3D simulations to date (making use of the AREPO code) in order to explore both direct and indirect collisions and the conditions in which they give rise to a detonation and the production of a luminous SNe. Using our simulations, we find a detonation criterion that can provide the critical impact parameter for an explosion to occur, depending on the density profile of the colliding WDs, their composition, and their collision velocities. We find that the initial velocity has a significant impact on the amount of 56Ni production from the explosion. Furthermore, the production of the 56Ni also depends on numerical modeling aspects.