Development of a low-background neutron detector array-Reference-Cited by-同舟云学术

Development of a low-background neutron detector array

Published:2022-04 Issue:4 Volume:33 Page:
ISSN:1001-8042
Container-title:Nuclear Science and Techniques
language:en
Short-container-title:NUCL SCI TECH

Author:

Li Yu-Tian^ORCID,Lin Wei-Ping^ORCID,Gao Bing-Shui,Chen Han,Huang Hao,Huang Yu,Jiao Tao-Yu,Li Kuo-Ang,Tang Xiao-Dong^ORCID,Wang Xin-Yu,Fang Xiao^ORCID,Huang Han-Xiong,Ren Jie^ORCID,Ru Long-Hui,Ruan Xi-Chao,Zhang Ning-Tao,Zhang Zhi-Chao

Publisher

Springer Science and Business Media LLC

Subject

Nuclear Energy and Engineering,Nuclear and High Energy Physics

Link

https://link.springer.com/content/pdf/10.1007/s41365-022-01030-0.pdf

Reference28 articles.

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2. B. Guo, Z.H. Li, M. Lugaro et al., New determination of the $$^{13}$$C($$\alpha$$, n)$$^{16}$$O reaction rate and its influence on the s-process nucleosynthesis in AGB stars. Astrophys. J. 756, 193–195 (2012). https://doi.org/10.1088/0004-637x/756/2/193

3. R.J. de Boer, C.R. Brune, M. Febrarro et al., Sensitivity of the $$^{13}{\rm C}({\alpha }, n)^{16}{\rm O}\,\, S$$ factor to the uncertainty in the level parameters of the near-threshold state. Phys. Rev. C 101, 045802 (2020). https://doi.org/10.1103/PhysRevC.101.045802

4. F. Herwig, M. Pignatari, P.R. Woodward et al., Convective-reactive proton-12C combustion in sakurais object(V4334 SAGITTARII) and implications for the evolution and yields from the first generations of stars. Astrophys. J. 727, 89 (2011). https://doi.org/10.1088/0004-637X/727/2/89

5. P. Banerjee, Y.-Z. Qian, A. Heger, New neutron-capture site in massive Pop III and Pop II stars as a source for heavy elements in the early galaxy. Astrophysical J. 865, 120 (2018). https://doi.org/10.3847/1538-4357/aadb8c

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