Experimental measurement of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Zr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>91</mml:mn></mml:mmultiscripts></mml:math> ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo>)</mml:mo><mml:mmultiscripts><mml:mi>Zr</mml:mi><mml:mprescripts/><mml:none/><mml:mn>92</mml:mn></mml:mmultiscripts></mml:mrow></mml:math> at the CSNS Back-n facility from 0.82 keV to 229 keV-Reference-Cited by-同舟云学术

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Experimental measurement of Zr91 ( n,γ)Zr92 at the CSNS Back-n facility from 0.82 keV to 229 keV

Published:2024-08-15 Issue:2 Volume:110 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Gan L.¹,Sun H. B.²²,Jiang W.³⁴⁵,Li Z. H.⁶⁷,Zhong J.⁸^ORCID,Rohilla A.⁹^ORCID,Huang Z. Y.¹⁰,Li X. Y.¹¹^ORCID,Nan W.⁶^ORCID,Nan W. K.⁶^ORCID,Hu S. P.²²,Li E. T.²

Affiliation:

1. Shenzhen Institute of Information Technology

2. Shenzhen University

3. Spallation Neutron Source Science Center

4. Institute of High Energy Physics

5. Chinese Academy of Sciences

6. China Institute of Atomic Energy

7. Jinping Deep Underground Frontier Science and Dark Matter Key Laboratory of Sichuan Province

8. Shenzhen Technology University

9. University of Nebraska-Lincoln

10. Origin Quantum Computing Technology (Hefei) Co., Ltd.

11. Fudan University

Funder

National Natural Science Foundation of China

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.110.025802/fulltext

Reference32 articles.

1. Synthesis of the Elements in Stars

2. s‐Process Nucleosynthesis in Asymptotic Giant Branch Stars: A Test for Stellar Evolution

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

4. Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components

5. Capitalizing on nuclear data libraries' comprehensiveness to obtain solar r-process abundances

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