Neutron capture cross section and capture <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>γ</mml:mi></mml:math> -ray spectrum of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Sr</mml:mi><mml:mprescripts /><mml:none /><mml:mn>88</mml:mn></mml:mmultiscripts></mml:math> in the stellar nucleosynthesis energy region-Reference-Cited by-同舟云学术

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Neutron capture cross section and capture γ -ray spectrum of Sr88 in the stellar nucleosynthesis energy region

Published:2023-09-11 Issue:3 Volume:108 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Katabuchi Tatsuya^ORCID,Igashira Masayuki,Kamada So,Tajika Michihide,Iwamoto Nobuyuki,Kawano Toshihiko^ORCID

Funder

Institute of Innovative Research, Tokyo Institute of Technology

U.S. Department of Energy

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.108.034610/fulltext

Reference25 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. Massive Stars in the Range 13–25 M ⊙ : Evolution and Nucleosynthesis. II. The Solar Metallicity Models

4. THE WEAKs-PROCESS IN MASSIVE STARS AND ITS DEPENDENCE ON THE NEUTRON CAPTURE CROSS SECTIONS

5. High-resolution neutron capture and transmission measurements, and the stellar neutron-capture cross section of88Sr

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