The double-degenerate model for the progenitors of type Ia supernovae
Dongdong Liu, Bo Wang, Zhanwen Han

TL;DR
This study models the double-degenerate pathway for type Ia supernovae, incorporating the WD+He subgiant channel, and finds it can reproduce observed rates and delay time distributions, with violent mergers contributing a minority.
Contribution
It introduces a detailed grid for WD+He star systems and demonstrates that including this channel aligns theoretical predictions with observations.
Findings
Galactic SNe Ia rate is about 2.4×10^{-3} yr^{-1} from the WD+He subgiant channel.
Total SNe Ia rate from all channels is approximately 3.7×10^{-3} yr^{-1}, matching observations.
Violent WD mergers contribute roughly 16% of all SNe Ia.
Abstract
The double-degenerate (DD) model, involving the merging of massive double carbon-oxygen white dwarfs (CO WDs) driven by gravitational wave radiation, is one of the classical pathways for the formation of type Ia supernovae (SNe Ia). Recently, it has been proposed that the WD+He subgiant channel has a significant contribution to the production of massive double WDs, in which the primary WD accumulates mass by accreting He-rich matter from a He subgiant. We evolved about 1800 CO WD+He star systems and obtained a large and dense grid for producing SNe Ia through the DD model. We then performed a series of binary population synthesis simulations for the DD model, in which the WD+He subgiant channel is calculated by interpolations in this grid. According to our standard model, the Galactic birthrate of SNe Ia is about 2.4*10^{-3} yr^{-1} for the WD+He subgiant channel of the DD model; the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
