Stellar evolution, SN explosion, and nucleosynthesis
K. Maeda. (2022)cite arxiv:2210.00326Comment: 42 pages, 17 figures; Invited chapter for Handbook of X-ray and Gamma-ray Astrophysics (Eds. C. Bambi and A. Santangelo, Springer Singapore, expected in 2022). References updated.
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.
Description
Stellar evolution, SN explosion, and nucleosynthesis
cite arxiv:2210.00326Comment: 42 pages, 17 figures; Invited chapter for Handbook of X-ray and Gamma-ray Astrophysics (Eds. C. Bambi and A. Santangelo, Springer Singapore, expected in 2022). References updated
%0 Generic
%1 maeda2022stellar
%A Maeda, Keiichi
%D 2022
%K astrophysics cosmology interesting review
%T Stellar evolution, SN explosion, and nucleosynthesis
%U http://arxiv.org/abs/2210.00326
%X 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.
@misc{maeda2022stellar,
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.},
added-at = {2023-01-01T13:37:27.000+0100},
author = {Maeda, Keiichi},
biburl = {https://www.bibsonomy.org/bibtex/20347329087657bbb0a2b8c27c434fa45/intfxdx},
description = {Stellar evolution, SN explosion, and nucleosynthesis},
interhash = {da39c35b9ed8d136849c866a35da4dca},
intrahash = {0347329087657bbb0a2b8c27c434fa45},
keywords = {astrophysics cosmology interesting review},
note = {cite arxiv:2210.00326Comment: 42 pages, 17 figures; Invited chapter for Handbook of X-ray and Gamma-ray Astrophysics (Eds. C. Bambi and A. Santangelo, Springer Singapore, expected in 2022). References updated},
timestamp = {2023-01-01T13:37:27.000+0100},
title = {Stellar evolution, SN explosion, and nucleosynthesis},
url = {http://arxiv.org/abs/2210.00326},
year = 2022
}