On the evolution of rotating accreting white dwarfs and type Ia supernovae

TL;DR

This study investigates how rotation affects the evolution of accreting white dwarfs in single-degenerate models of type Ia supernovae, revealing a higher proportion of explosions supported by solid-body rotation and exploring diversity origins.

Contribution

It provides a detailed binary population synthesis analysis considering rotation, highlighting the impact on white dwarf mass distribution and supernova diversity in the single-degenerate channel.

Findings

77% of SNe Ia explode with WD masses supporting solid-body rotation

Only 2% have WD masses >2.0Msun, requiring larger initial WD mass

Some progenitors with circumstellar hydrogen may involve differential rotation

Abstract

The potential importance of the angular momentum which is gained by accreting white dwarfs (WDs) has been increasingly recognized in the context of type Ia supernova (SN Ia) single-degenerate model. The expectation that the spin of the WD can delay the explosion should help the single-degenerate model to be consistent with the observed properties of most SNe Ia, in particular by avoiding hydrogen contamination. In this article, we attempt to study the most prominent single-degenerate supersoft (WD + MS) channel when the rotation of accreting WDs is considered. We present a detailed binary population synthesis study to examine the predicted population of SNe Ia for this channel. For our standard model, we find that 77% of these SNe Ia explode with WD masses which are low enough to be supported by solid-body rotation (1.378-1.5Msun); this is a substantially higher proportion than found by previous work. Only 2% have WD explosion masses >2.0Msun; these require the initial WD mass to be larger than 1.0 Msun. We further discuss the possible origin of the diversity of SNe Ia from the pre- and post- accretion properties of the WDs in this population. We also suggest that some SN Ia progenitors with substantial circumstellar hydrogen, including some apparent type IIn SNe, might be related to WDs which required support from differential rotation to avoid explosion, since these can still be accreting from hydrogen-rich donors with a relatively high mass-transfer rate at the time of the SN explosion.