Contribution of the \(M1\) process to the astrophysical \(S\)-factor of the \(p^{2}\)H radiative capture

DOI10.1007/S11182-011-9593-4zbMath1235.81125OpenAlexW2011145737MaRDI QIDQ664948

S. B. Dubovichenko

Publication date: 5 March 2012

Published in: Russian Physics Journal (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11182-011-9593-4

zbMATH Keywords

cluster modelastrophysical \(S\)-factorslight atomic nucleilow energyphotonuclear processesthermonuclear reactions

Mathematics Subject Classification ID

Nuclear physics (81V35) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (1)

Phase analysis of \(n^{12}\mathrm{C}\) elastic scattering at low energies

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