Nucleosynthesis in metal-free and metal-poor stars

Yong Zhong Qian

doi:10.1063/1.2905564

Nucleosynthesis in metal-free and metal-poor stars

Yong Zhong Qian

Physics and Astronomy (Twin Cities)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

There have been a number of important recent developments in theoretical and observational studies of nucleosyn-thesis, especially regarding nucleosynthetic sources at low metallicities. Those selected for discussion here include the origin of ⁶Li, the primary production of N, the s-process, and the supernova sources for three groups of metals: (1) C to Zn with mass numbers A<70, (2) Sr to Ag with A∼90-110, and (3) r-process nuclei with A∼130 and above.

Original language	English (US)
Title of host publication	First Stars III
Pages	283-290
Number of pages	8
DOIs	https://doi.org/10.1063/1.2905564
State	Published - 2008
Event	First Stars III - Santa Fe, NM, United States Duration: Jul 15 2007 → Jul 20 2007

Publication series

Name	AIP Conference Proceedings
Volume	990
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	First Stars III
Country/Territory	United States
City	Santa Fe, NM
Period	7/15/07 → 7/20/07

Keywords

Abundances
Neutrinos
Nucleosynthesis
Supemovae

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10.1063/1.2905564

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abstract = "There have been a number of important recent developments in theoretical and observational studies of nucleosyn-thesis, especially regarding nucleosynthetic sources at low metallicities. Those selected for discussion here include the origin of 6Li, the primary production of N, the s-process, and the supernova sources for three groups of metals: (1) C to Zn with mass numbers A<70, (2) Sr to Ag with A∼90-110, and (3) r-process nuclei with A∼130 and above.",

keywords = "Abundances, Neutrinos, Nucleosynthesis, Supemovae",

author = "Qian, {Yong Zhong}",

year = "2008",

doi = "10.1063/1.2905564",

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series = "AIP Conference Proceedings",

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AB - There have been a number of important recent developments in theoretical and observational studies of nucleosyn-thesis, especially regarding nucleosynthetic sources at low metallicities. Those selected for discussion here include the origin of 6Li, the primary production of N, the s-process, and the supernova sources for three groups of metals: (1) C to Zn with mass numbers A<70, (2) Sr to Ag with A∼90-110, and (3) r-process nuclei with A∼130 and above.

KW - Abundances

KW - Neutrinos

KW - Nucleosynthesis

KW - Supemovae

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T2 - First Stars III

Y2 - 15 July 2007 through 20 July 2007

ER -

Nucleosynthesis in metal-free and metal-poor stars

Abstract

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