The -process in the carbon deflagration model for type Ia supernovae and chronology of the solar system formation

Kusakabe, Motohiko*; Iwamoto, Nobuyuki ; Nomoto, Kenichi*

We consider nucleochronology with four -process radioactive nuclides $^{53}$ Mn, $^{92}$ Nb, $^{97}$ Tc and $^{146}$ Sm which are produced in a carbon deflagration model for type Ia supernovae. We apply the result of the -process nucleosynthesis to simple galactic chemical evolution models and discuss the circumstances of the solar system formation.

Language	:	English
Journal	:	AIP Conference Proceedings 847
Volume	:
Number	:
Pages	:	p.424 - 426
Publication Year/Month	:	2006/07
Meeting title	:	International Symposium on Origin of Matter and Evolution of Galaxies 2005 (OMEG '05)
Held date	:	2005/11
Location (city)	:	Tokyo
Location (country)	:	Japan
Patent information	:
PDF	:
Paper URL	:	https://doi.org/10.1063/1.2234446
DOI for research data	:
Keywords	:	no keyword
Research Facility	:
Press Release	:
Article of JAEA R&D Review	:
Cooperating Institute	:

Accesses	:	- Accesses
Web of Science® Times Cited Count	:	Times Cited Count： If you would like to get the latest times cited, please access the Web of Science®. http://www.webofknowledge.com/wos
InCites™	:
Altmetrics	:

Registration No. : BB20050876
JAEA Abstracts No. : 34001010
Paper Submission No. : 1155

[CLARIVATE ANALYTICS], [WEB OF SCIENCE], [HIGHLY CITED PAPER & CUP LOGO] and [HOT PAPER & FIRE LOGO] are trademarks of Clarivate Analytics, and/or its affiliated company or companies, and used herein by permission and/or license.