Supernovae Ia in 2019 (review): a rising demand for spherical explosions
Noam Soker (Technion, Israel)

TL;DR
This review highlights that most normal Type Ia supernovae are spherical explosions, mainly arising from specific scenarios like the Chandrasekhar mass WD explosion, while others produce peculiar, non-spherical events.
Contribution
The paper synthesizes recent 2019 studies to clarify which SN Ia progenitor scenarios produce spherical versus peculiar explosions, emphasizing the importance of explosion symmetry.
Findings
Most normal SNe Ia are globally spherical with possible clumps.
Dynamical explosion scenarios tend to produce non-spherical, peculiar SNe Ia.
Chandrasekhar mass WD explosions align with observations of normal SNe Ia.
Abstract
I review new studies of type Ia supernovae (SNe Ia) from 2019, and use these to improve the comparison between the five binary SN Ia scenarios. New low polarisation measurements solidify the claim that most SN Ia explosions are globally spherically symmetric (clumps are possible). Explosions by dynamical processes, like explosions that take place during a merger process of two white dwarfs (WDs) in the double degenerate (DD) scenario, or during an accretion process in the double detonation (DDet) scenario and in the single degenerate (SD) scenario, lead to non-spherical explosions, in contradiction with observations of normal SNe Ia. I argue that these (DD, DDet, SD) scenarios account mainly for peculiar SNe Ia. The explosion of a Chandrasekhar mass (Mch) WD (deflagration to detonation process) has a global spherical structure that is compatible with observations. To reach spherical…
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.
