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Asymptotic normalization coefficient method for two-proton radiative capture
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DOI：10.1016/j.physletb.2020.135852.png)
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摘要
En 中文
The method of asymptotic normalization coefficients is a standard approach for studies of two-body non-resonant radiative capture processes in nuclear astrophysics. This method suggests a fully analytical description of the radiative capture cross section in the low-energy region of the astrophysical interest. We demonstrate how this method can be generalized to the case of three-body 2p radiative captures. It was found that an essential feature of this process is the highly correlated nature of the capture. This reflects the complexity of three-body Coulomb continuum problem. Radiative capture O-15+p+p -> Ne-17+gamma is considered as an illustration. (C) 2020 The Author(s). Published by Elsevier B.V.
Keyword:
Asymptotic normalization coefficient method
Two-proton nonresonant radiative capture
E1 strength function
Three-body hyperspherical harmonic method
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期刊
IF:
4.5
论文数:
3.2W
被引数:
7.3W
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