Re-examination of astrophysical S-factor of proton capture Be9(p,γ)10B in stellar matter
Author:
Funder
Higher Education Commission, Pakistan
Publisher
Elsevier BV
Subject
Nuclear and High Energy Physics
Reference27 articles.
1. On the Origin of Light Elements
2. Abundances of the elements: Meteoritic and solar
3. Study of the nucleon radiative captures 8Li(n,γ)9Li, 9Be(p,γ)10B, 10Be(n,γ)11Be, 10B(p,γ)11C, and 16O(p,γ)17F at thermal and astrophysical energies
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1. Re-analysis of temperature dependent neutron capture rates and stellar β-decay rates of 95-98Mo;Chinese Physics C;2024-09-01
2. The astrophysical S factor of p+9Be radiative capture reaction in a potential model;New Astronomy;2024-05
3. Re-investigation of Neutron Capture by $$^{84}$$Kr and $$^{86}$$Kr in the s-Process Nucleosynthesis;Brazilian Journal of Physics;2024-03-27
4. Investigation of 90,92Zr(n,γ)91,93Zr in the s-process nucleosynthesis;Zeitschrift für Naturforschung A;2024-02-19
5. The Thermonuclear Rate of $${}^{\mathbf{9}}\mathbf{Be}$$($$\mathbf{p}$$, $$\boldsymbol{\gamma}$$)$${}^{\mathbf{10}}$$B Reaction by Using the Modified Potential Model*;Astronomy Letters;2023-11
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