Stellar evolution, SN explosion, and nucleosynthesis

TL;DR

This paper reviews the evolution of massive stars and white dwarfs leading to supernova explosions, discussing mechanisms, nucleosynthesis, and observational constraints to understand these catastrophic stellar events.

Contribution

It provides a comprehensive overview of stellar evolution pathways, explosion mechanisms, and nucleosynthesis processes, integrating recent observational data to address unresolved problems.

Findings

Different supernova types linked to specific stellar evolution channels

Explosion mechanisms characterized for various supernova classes

Observational properties used to constrain progenitor models

Abstract

Massive stars evolve toward the catastrophic collapse of their innermost core, producing core-collapse supernova (SN) explosions as the end products. White dwarfs, formed through evolution of the less massive stars, also explode as thermonuclear SNe if certain conditions are met during the binary evolution. Inflating opportunities in transient observations now provide an abundance of data, with which we start addressing various unresolved problems in stellar evolution and SN explosion mechanisms. In this chapter, we overview the stellar evolution channels toward SNe, explosion mechanisms of different types, and explosive nucleosynthesis. We then summarize observational properties of SNe through which the natures of the progenitors and explosion mechanisms can be constrained.