Probing astrophysically important states in theMg26nucleus to study neutron sources for thesprocess-Reference-Cited by-同舟云学术

Probing astrophysically important states in theMg26nucleus to study neutron sources for thesprocess

Published:2016-05-10 Issue:5 Volume:93 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Talwar R.,Adachi T.,Berg G. P. A.,Bin L.,Bisterzo S.,Couder M.,deBoer R. J.,Fang X.,Fujita H.,Fujita Y.,Görres J.,Hatanaka K.,Itoh T.,Kadoya T.,Long A.,Miki K.,Patel D.,Pignatari M.,Shimbara Y.,Tamii A.,Wiescher M.,Yamamoto T.,Yosoi M.

Funder

National Science Foundation

Magyar Tudományos Akadémia

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Partnership for Advanced Computing in Europe AISBL

Commonwealth Scholarship Commission

Kungliga Tekniska Högskolan

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.93.055803/fulltext

Reference89 articles.

1. Thesprocess: Nuclear physics, stellar models, and observations

2. S-process nucleosynthesis in massive stars and the weak component. II - Carbon burning and galactic enrichment

3. Evolution and Nucleosynthesis in Low‐Mass Asymptotic Giant Branch Stars. II. Neutron Capture and thes‐Process

4. Neutron-Capture Elements in the Early Galaxy

5. What are the astrophysical sites for the r-process and the production of heavy elements?

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