Measurement of Br(n,γ) cross sections up to stellar s-process temperatures at the CSNS Back-n
Author:
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/s41365-023-01337-6.pdf
Reference55 articles.
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2. P.A. Egelstaff, B.T. Taylor, Slow neutron cross-sections of molybdenum and bromine. Nature 166, 825 (1950). https://doi.org/10.1038/166825b0
3. M. Heil, M. Pignatari, The weak s-process and its relation to explosive nucleosynthesis. In AIP Conferences Proceedings. vol. 819, p. 265 (2006). https://doi.org/10.1063/1.2187869
4. S.E. Woosley, W.A. Fowler, J.A. Holmes et al., Semiempirical thermonuclear reaction-rate data for intermediate-mass nuclei. At. Data Nucl. Data Tables 22, 371 (1978). https://doi.org/10.1016/0092-640x(78)90018-9
5. M. Heil, F. Käppeler, E. Uberseder et al., Stellar (n,$$\gamma $$) cross sections for Br and Rb: matching the weak and mains-process components. Phys. Rev. C 78, 025802 (2008). https://doi.org/10.1103/PhysRevC.78.025802
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