Type Ia Supernovae: Can Coriolis force break the symmetry of the gravitational confined detonation explosion mechanism?
D. Garc\'ia-Senz, R.M. Cabez\'on, I. Dom\'inguez, F.K. Thielemann

TL;DR
This study investigates how rotation and the Coriolis force influence the symmetry and effectiveness of the gravitational confined detonation mechanism in Type Ia supernovae, suggesting rotation may hinder detonation development.
Contribution
It demonstrates that rotation can break symmetry in the explosion mechanism, potentially challenging the viability of the gravitational confined detonation model for Type Ia supernovae.
Findings
Rotation affects the symmetry of the deflagration process.
The Coriolis force weakens the convergence of the nuclear flame.
Rotation may prevent detonation in the gravitational confined mechanism.
Abstract
Nowadays the number of models aimed at explaining the Type Ia supernova phenomenon is high and discriminating between them is a must-do. In this work we explore the influence of rotation in the evolution of the nuclear flame which drives the explosion in the so called gravitational confined detonation models. Assuming that the flame starts in a point-like region slightly above the center of the white dwarf (WD) and adding a moderate amount of angular velocity to the star we follow the evolution of the deflagration using a smoothed particle hydrodynamics code. We find that the results are very dependent on the angle between the rotational axis and the line connecting the initial bubble of burned material with the center of the white dwarf at the moment of the ignition. The impact of rotation is larger for angles close to 90{\deg} because the Coriolis force on a floating element of fluid…
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